The galaxy presents a smooth, largely featureless morphology. It exhibits a centrally concentrated light distribution, suggestive of a significant bulge component. The galaxy's shape appears largely round. There is no obvious spiral arm structure or bar. The color gradient suggests the core is somewhat older, and redder, than the regions surrounding it. There is little evidence of recent or ongoing major merging activity. A slight asymmetry in the outer regions might indicate a minor interaction or past disturbance, however. Star formation is expected to be minimal within this galaxy.
