The galaxy presents as a primarily smooth, elliptical-like structure. Its core appears bright and concentrated, with a yellow hue. This suggests a population of older stars dominating the central region. The light gradually diffuses outwards from the core. There is evidence of very faint extensions or tidal tails visible in the outer regions, indicative of past or ongoing interactions. The galaxy appears largely isolated, with no other interacting galaxies in close proximity. The overall color profile suggests a relatively low star formation rate. The galaxy exhibits a slight elongation, deviating minimally from a perfectly circular shape. There appears to be some minor disturbance in the galaxy.
