The galaxy appears to be a relatively smooth, round structure. It exhibits a concentrated central bulge, yellow-white in color, that gradually fades into a more diffuse, fainter halo. The overall color suggests an older stellar population, potentially indicating a lower rate of star formation. There are no visible spiral arms or significant dust lanes present. There may be some very minor disturbances that are hard to distinguish. The galaxy's morphology is broadly consistent with an elliptical galaxy type, possibly transitioning into a lenticular one.
