The galaxy presents a smooth, elliptical morphology. It displays a concentrated central bulge that gradually fades into the outer regions. The color gradient suggests an older stellar population dominating the light emission, particularly in the central region. There is little indication of spiral arms or significant dust lanes. A faint, diffuse halo might extend beyond the main body, but it is difficult to discern due to its faintness and the background noise. The overall appearance is consistent with a relatively quiescent galaxy, lacking significant ongoing star formation. There is no sign of tidal tails or other major disturbances indicative of recent mergers, although there might be slight irregularities in the outer edges.
