The galaxy presents as an elliptical or lenticular type, characterized by a smooth, centrally concentrated light profile. It exhibits a somewhat elongated, cigar-like shape rather than a perfectly circular appearance. There is a noticeable absence of distinct spiral arms or a prominent disk structure. The central region shows a bright, yellowish-white hue, potentially indicative of an older stellar population. Marginal disturbances are present, but there is no evidence of a major merger in progress, nor distinct tidal tails or strong asymmetry in the galactic structure. The average rate of star formation is low. The galaxy has a high mass. 