The galaxy presents as a slightly elongated, centrally concentrated object. The light distribution suggests a dominant spheroidal component, exhibiting a smooth, diffuse profile. The core region appears brighter and more yellow, suggestive of an older stellar population with less active star formation. Extending outwards, a bluer halo is observed, indicating a younger stellar population and the potential for ongoing or recent star formation activity. There is a subtle indication of a possible disk component, but its structure appears relatively undisturbed, with only faint, almost imperceptible asymmetries in the outer regions. The galaxy's red color is prominent, suggesting an evolved stellar population overall. There's no obvious evidence of strong tidal interactions or major disturbances. It appears to be a relatively isolated galaxy.
