The galaxy presents as a slightly elongated, lenticular-like structure with a relatively smooth appearance. A bright, concentrated central bulge dominates the morphology, exhibiting a yellowish-white hue, possibly indicative of an older stellar population. Fainter, diffuse light extends outwards from the bulge, forming a flattened disk-like structure. This disk is characterized by a reddish tint, suggestive of a mix of older stars and dust lanes. The overall shape is neither perfectly round nor highly elongated; it exhibits an intermediate form. There is no strong evidence of a major ongoing merger, though subtle distortions might indicate a past interaction or minor disturbances. The galaxy shows no signs of active star formation regions. The overall color profile indicates a galaxy that is transitioning from a more active, star-forming state to a more quiescent one.
