The galaxy appears as a moderately bright, elliptical or lenticular system. The light is concentrated towards the center, suggesting a prominent bulge. The galaxy exhibits a smooth light distribution with little visible substructure, indicating a lack of spiral arms. The primary color is yellowish, likely indicative of an older stellar population. Faint bluish regions are observed surrounding this yellower core, indicating possible recent star formation. There does not appear to be any evidence of significant tidal disturbances or ongoing merger activity. The overall morphology suggests a relatively evolved system.
