The galaxy presents as a luminous, elongated object. It exhibits a generally smooth morphology, with a concentrated central bulge that graduates into a more diffuse disk. The major axis is approximately three times the length of the minor axis. The color profile suggests a moderate amount of ongoing star formation within the disk, indicated by the bluish tint, whereas the central bulge appears more yellow, potentially indicating an older stellar population. There is no indication of a strong spiral structure, but the disk does show some faint hints of substructure. No significant tidal features or close companions are apparent, suggesting the galaxy is relatively undisturbed. There is a possibility of a minor disturbance within the galaxy based on the image.
