The galaxy presents as a relatively compact, elliptical-like structure. Its core exhibits a bright, concentrated luminosity. The central region appears predominantly smooth, lacking distinct spiral arm features or prominent dust lanes. The overall color profile suggests a population of older stars, with a discernible redder hue towards the outer edges of the galaxy, in contrast with bluer stars located towards the center. There may be a faint, extended halo surrounding the main body, but its visibility is limited. The object appears generally undisturbed, with no major signs of recent or ongoing merger activity.
