The galaxy presents as a somewhat smooth, centrally concentrated object. There is a dominant, bright central bulge that exhibits a yellow to golden hue, suggesting a population of older stars. Fainter, diffuse light extends outwards from the core in a somewhat elliptical shape, which is not perfectly round, and instead slightly elongated. The outer regions show hints of bluer colors, indicating the presence of younger stars. There is no clear evidence of spiral arm structure or a well-defined disk. There are no strong indications of tidal tails or obvious signs of a major ongoing merger event. The galaxy appears relatively undisturbed, although there are some minor irregularities in the outer regions, indicative of possibly past interactions. Star formation activity appears to be relatively low, based on the color distribution.