The galaxy presents as a relatively smooth, elliptical-like structure. It appears to be somewhat rounded in shape, with minimal discernible features suggesting a disk or spiral arms. The color profile exhibits a concentration of yellowish-orange hues towards the central region, possibly indicative of an older stellar population. The outer regions display a subtle shift towards a more greenish-blue tint, suggesting the presence of at least some younger stars. There are no obvious signs of a major ongoing merger or significant tidal disturbances in the surrounding region, although there is a hint of asymmetry at the lower edge of the galaxy. The galaxy's diffuse glow indicates the presence of a substantial stellar component.
