The galaxy presents as a centrally concentrated object with a smooth, elliptical morphology. A slight color gradient is visible, with the central region appearing more reddish in hue, gradually transitioning to bluer tones towards the outer edges. This suggests a possible difference in stellar population, with older, redder stars dominating the core and younger, bluer stars populating the outskirts. The overall structure exhibits a high degree of symmetry, indicating a relaxed dynamical state. There is no noticeable presence of spiral arms, bars, or significant dust lanes. Faint, diffuse light extends outwards, suggesting a halo of stars surrounding the main galactic body. The absence of prominent tidal features argues against recent major merger events, though minor disturbances cannot be ruled out. The galaxy appears largely undisturbed and relatively isolated.
