The galaxy exhibits a flattened, elliptical morphology, appearing somewhat cigar-shaped from this viewing angle. A dominant central bulge is evident, displaying a yellowish hue, suggestive of an older stellar population. Fainter, bluer regions extend outward from the central bulge, particularly on the left side of the image. These bluer regions imply the presence of younger stars and potentially ongoing star formation, though at a low rate. The galaxy lacks a clearly defined spiral structure or prominent dust lanes, indicating it's likely an early-type spiral or a lenticular galaxy nearing the end of its spiral structure. There is a hint of disturbance or tidal features, though no significant merger or major distortion is evident.
