The galaxy presents as a somewhat inclined disk galaxy with a moderate degree of internal structure. Its shape is elongated, suggesting an elliptical appearance when viewed from Earth. The galactic disk exhibits a mottled texture, with regions of intense blue light interspersed with areas of more diffuse, yellowish light. These brighter blue regions likely indicate areas of active star formation, while the yellower areas may be indicative of older stellar populations.

There is some evidence of a faint central bulge, but the bulge is not particularly prominent. The overall appearance of the galaxy suggests a relatively low surface brightness with some star formation in the disk, but not intense widespread activity. There appears to be a slight warping or disturbance of the galactic disk on one side. The image does not show a strong spiral structure, but there are irregularities throughout the disk, as if it might be a barred spiral galaxy but without clearly defined arms, or simply an irregular disk galaxy. No apparent tidal tails or signs of interaction with a companion galaxy are visible in this image, however, this does not exclude the possibility of past or ongoing mergers, especially given the aforementioned warp.
