The galaxy presents as a relatively smooth, elliptical-type structure with a concentrated central bulge. Its overall color profile appears yellow-red, suggesting a population dominated by older stars and a lower rate of ongoing star formation. There is little evidence of significant spiral arm structure or prominent dust lanes. The galaxy appears isolated, showing no strong indications of tidal interactions or recent merger events, although there may be a slight asymmetry or minor disturbance on one side. The galaxy's profile is generally round, with a slight deviation towards an intermediate shape.
