The galaxy appears to be a relatively smooth, elliptical system with a concentrated central bulge. The light distribution exhibits a fairly uniform gradient outward from the core, with no apparent spiral arm structures or distinct features. The overall color profile tends toward redder hues, potentially indicative of an older stellar population. The galaxy's shape is generally round. There's no visual evidence suggesting ongoing or recent major merging activity, although subtle asymmetries may hint at minor tidal interactions.
