The galaxy presents a largely smooth morphology, appearing elliptical in shape, with a high degree of roundness. There is a concentrated central bulge that is yellow-orange in color, indicating a likely older stellar population. Faint disk-like or spiral features are possibly embedded within the diffused outer edges, though difficult to discern with certainty. The overall color suggests a lack of significant recent star formation. Evidence shows that this galaxy is not undergoing any significant merging events.
