The galaxy exhibits a predominantly smooth morphology, suggesting an elliptical classification, though a subtle disk-like feature may be present. It presents an oblate spheroidal shape, neither perfectly round nor significantly elongated. The galaxy's light profile appears relatively concentrated, with a bright central bulge and a gradually fading outer halo. There is no strong evidence of ongoing major merger activity, although some minor disturbances may be present. The galaxy's color is primarily yellowish-white, indicating a stellar population dominated by older stars, but with some suggestion of recent star formation.
