The galaxy presents a generally smooth morphology, appearing somewhat elliptical in shape. There is a bright, concentrated central bulge or nucleus, suggesting a significant population of older stars and potentially a supermassive black hole at its core. Fainter, diffuse light extends outward from the central region, forming a halo of stars and dust. The galaxy exhibits a color gradient, with the core appearing bluer or whiter, indicative of younger, hotter stars or active galactic nucleus activity, while the outer regions appear redder, suggesting an older stellar population. There appears to be some asymmetry in the outer regions of the galaxy, hinting at potential tidal interactions or past merger events. The disk, if present, is not clearly defined, and it doesn't appear to have spiral arm structure. The galaxy shows some signs of disturbance, with an irregularity in the outer halo on one side.
