This galaxy appears to be a relatively smooth, elliptical galaxy. It exhibits a concentrated central bulge that fades gradually into an extended halo. The overall color profile suggests a stellar population dominated by older, redder stars, as indicated by the yellowish-white hue, with a possible contribution from dust. No distinct spiral arms or prominent dust lanes are visible. There is a slight asymmetry, possibly due to a minor tidal interaction or internal kinematic effects. The morphology is primarily smooth, and the overall shape suggests that the galaxy is viewed close to face-on, despite the somewhat elongated appearance. The galaxy shows no signs of a major ongoing merger.
