The galaxy presents as a roughly elliptical, yellowish-white object. The light is centrally concentrated, suggesting a large bulge component with a higher density of older stars. There is only the slightest hint of a disk and little evidence of spiral arm structure. It appears moderately luminous. Faint color variations exist across the galaxy, but no strong blue star formation regions are visible. The overall morphology suggests a relatively smooth light distribution, which could indicate that this is an older galaxy with a declining star formation rate. There is no clear sign of a major merger or tidal disturbances.
