The galaxy presents as a slightly elongated, diffuse object. It exhibits a centrally concentrated luminosity profile, with a smooth appearance, suggesting an elliptical morphology or a spiral galaxy viewed at a high inclination. There are no distinct spiral arm structures visible. The galaxy's light is primarily distributed in a fairly uniform manner, lacking strong color gradients or prominent features such as dust lanes or star-forming regions. The color is subtly bluer in the central region fading to redder hues towards the outer edges, which implies older stellar populations are more dominant in the outer regions. The overall light distribution indicates a relatively quiescent galaxy with a low star formation rate. There are no obvious signs of a major ongoing merger or tidal disturbances.
