The galaxy presents a generally smooth morphology, suggesting it is likely an elliptical galaxy. It exhibits a bright central bulge that fades gradually towards the outer regions. The light distribution appears largely homogeneous, although there is a slight asymmetry possibly caused by a minor disturbance or interaction. The color gradient suggests an older stellar population, and the estimated size indicates that this is a relatively large galaxy. Star formation appears to be largely suppressed, and the overall structure suggests that it has likely undergone past merging events. The shape is neither perfectly round nor cigar-shaped, but rather falls somewhere in between.
