The galaxy appears as a relatively smooth, centrally concentrated object. It exhibits an elliptical morphology, with a high degree of central concentration as indicated by the brighter central region that gradually fades towards the outer edges. No distinct features such as spiral arms, bars, or prominent dust lanes are visible. There is a suggestion of bluer hues in the central region, transitioning to redder colors in the outer parts of the galaxy. This color gradient suggests the presence of a younger stellar population in the core, with older, redder stars populating the outer regions. The galaxy does not show any obvious signs of recent major merger activity or tidal disturbances.
