The galaxy in the image appears to be a relatively smooth, elliptical galaxy. It exhibits a concentrated central bulge that gradually fades into a more diffuse halo. There is little evidence of spiral arms or dust lanes, suggesting it is a more evolved system. The galaxy has a yellowish hue, potentially indicating an older stellar population dominated by redder stars. Its shape is nearly circular. There is no apparent ongoing major merger activity or significant tidal disturbances. The galaxy is compact, with a semi-major axis of approximately 2.9 kpc.
