The galaxy presents as an elliptical morphology, elongated along a principal axis, with a high degree of smoothness observed. The central region exhibits a bright, concentrated core, indicative of a spheroidal component. The galaxy displays a color gradient, with a bluer hue observed in the outer regions transitioning to a redder and potentially older stellar population in the core. There is a slight hint of possible disturbance or faint tidal features, but further observations are needed to confirm. The galaxy does not appear to be undergoing a major merger or significant star formation activity.
