The galaxy appears to be a relatively smooth, elliptical galaxy, exhibiting a largely featureless morphology. It has a generally rounded shape with a high degree of central concentration. The core region displays a yellowish hue, potentially indicating an older stellar population. There are faint traces of bluer light around the outer edges, which could represent some continuing, though subdued, star formation activity. There is no readily apparent evidence of ongoing mergers or major disturbances, with no substantial tidal tails or asymmetries. The galaxy appears relatively isolated, presenting as a well-formed single object.
