The galaxy presents a generally smooth, elliptical morphology. The central region exhibits a concentrated, bright core, indicative of a high stellar density. The color gradient suggests a population of older stars dominating the core, possibly due to a lack of recent star formation in that area. The outer regions fade gradually into the background, forming a diffuse halo. There are no visible spiral arms or significant dust lanes. The overall structure appears undisturbed, with no obvious signs of recent major mergers or tidal interactions, though there may be very minor disturbances. The round shape suggests a relatively relaxed dynamical state.
