The galaxy presents a predominantly disk-like morphology, viewed at a significant inclination. The central region exhibits a concentrated bulge of light, appearing with a yellowish hue, suggestive of an older stellar population. Extending outwards from the bulge, the disk displays a bluer color, indicating the presence of younger, hotter stars and active star formation. The galaxy does not appear perfectly smooth, revealing some underlying structure that may be indicative of spiral arms or irregular features within the disk. There may be signs of minor disturbance or ongoing interactions, though no significant merger is evident at this scale.
