The galaxy appears to be a relatively smooth, elliptical system. It exhibits a centrally concentrated brightness profile, with light gradually fading towards the outer regions. The shape is generally rounded, showing minimal deviation from a circular form. There is no indication of spiral arms, bars, or significant dust lanes. A slight asymmetry or minor disturbance might be present in its outer halo, but it's not clearly indicative of a major merging event. The overall color of the galaxy appears to be slightly blueish-white, suggesting the presence of some younger stars or ongoing star formation, though the galaxy is dominated by older stellar populations. The core displays brighter luminosity, and the outer edges are less distinct.