The galaxy appears as a relatively compact object, exhibiting a slightly elongated morphology. The central region displays a bright, concentrated core.  There is some indication of a faint, diffuse structure extending outward from the central region, appearing somewhat disturbed and asymmetrical.  A slight irregularity in the outer reaches could suggest a minor gravitational interaction or past merger event. Color gradients suggest that the outer regions are composed of a population of older stars, with the central area demonstrating the presence of some younger population of stars. There is indication of some dust lanes within the galaxy structure.
