The galaxy presents as a lenticular or early-type spiral galaxy with a generally smooth appearance. A faint disk-like structure is subtly visible, with a bright, concentrated bulge indicative of an older stellar population. The galaxy exhibits a redder hue in its central region, which then transitions to a bluer color towards the outer edges of its disk. The galaxy shows little signs of major disturbances or ongoing mergers with other galaxies. There is a slight elongation and is not perfectly round, it appears to be an intermediate shape. Star formation is estimated to be occurring at a very low rate. Overall, the galaxy appears relatively undisturbed and mature.
