The galaxy presents a generally smooth morphology, with a central bulge that is the brightest and most prominent feature. The galaxy exhibits a slightly elongated shape. There may be evidence of a weak disk structure, but it appears largely featureless. The color of the galaxy is indicative of an older stellar population, with a noticeable lack of bright blue stars, suggesting low ongoing star formation. Faint, diffuse light extends outwards from the main body, potentially indicating a stellar halo. There is a hint of asymmetry in the outer regions, possibly due to tidal interactions or past minor mergers, although no strong tidal tails are evident. The overall structure suggests a relatively relaxed system that is in the process of evolving towards a more quiescent state.