This galaxy presents as a relatively smooth, elliptical-like structure, with a bright, concentrated central bulge. The light distribution suggests a primarily older stellar population in the bulge, indicated by the redder hues compared to the faint disk. Some bluer color exists which suggests a low level of ongoing star formation. The galaxy exhibits a slight deviation from perfect roundness, appearing somewhat elongated. There are no readily apparent signs of major tidal disturbances or ongoing mergers, although a slight asymmetry in the outer regions might hint at minor interactions. The overall morphology is consistent with a galaxy that has largely completed its major assembly, and is slowly evolving.
