The galaxy presents as a relatively smooth, elliptical-like structure. The core is a bright, concentrated region exhibiting a yellow-white hue, indicating a population of older stars. Moving outward from the core, the light becomes less concentrated and transitions to a bluer color, possibly indicating the presence of a younger stellar population. The overall shape is moderately elongated, appearing somewhat cigar-shaped, with no distinct spiral arm structures or significant dust lanes visible. There is a slight suggestion of minor disturbances or tidal features surrounding the main body, hinting at past or ongoing gravitational interactions. No clear signs of a major merger are apparent.
