The galaxy appears to be a single, relatively smooth object with a concentrated central region. The overall color is yellowish-orange, suggesting an older stellar population with ongoing star formation. The galaxy exhibits a generally elliptical morphology with no obvious spiral arm structure or significant dust lanes visible. It is moderately luminous, but lacks evidence of any major ongoing merger activity or tidal disturbances. The galaxy is consistent with a lenticular or elliptical classification, leaning towards a system dominated by older stars.
