The galaxy presents a roughly elliptical morphology. It displays a bright, concentrated central bulge that appears slightly elongated along its major axis. This core region exhibits a reddish-white hue, suggesting a population of older stars.

Surrounding the central bulge, a diffuse disk component extends outwards. The disk exhibits a bluer color profile compared to the core, possibly indicating the presence of younger, hotter stars and ongoing star formation. The disk appears relatively smooth, with no readily discernible spiral arm structures or prominent dust lanes. There seems to be a faint, extended halo of light surrounding the main body of the galaxy, which could be composed of older stars or diffuse gas.

Overall, the galaxy's light distribution seems relatively smooth and centrally concentrated. There's no evidence of any strong tidal features or asymmetries, although there may be minor distortions present. These distortions could possibly be due to interactions with other galaxies.
