The galaxy presents as a relatively smooth, elliptical-like structure with no discernible spiral arms or bar features. Its morphology appears mostly uniform, dominated by a central bulge which emits a yellowish-orange light, indicative of an older stellar population. There is some indication of a slight extension beyond the core, giving a somewhat elongated appearance. There are hints of bluer light peripherally, suggesting the presence of some younger stars in the outer regions, however, this is less pronounced than the redder central bulge. There is no obvious sign of major mergers or tidal disturbances.
