The galaxy appears to be an elliptical galaxy, characterized by a relatively smooth and featureless morphology. It exhibits a concentrated central bulge that gradually fades into an extended halo. The light distribution appears round, with a noticeable decrease in brightness with increasing radius from the core. The galaxy displays a yellowish-orange hue centrally, suggesting an older stellar population dominates the core. There is a hint of bluer light in the outer regions, indicating the presence of some younger stars or ongoing star formation activity, although at a low rate. No distinct spiral arms or dust lanes are visible. There is no apparent evidence of a major merger event. The overall appearance suggests a quiescent system which may have experienced only minor disturbances or interactions in its recent history.
