The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge. The light distribution appears largely homogenous, lacking distinct spiral arms or significant dust lanes. The galaxy exhibits a yellow-white hue, suggesting a population of older stars dominating its stellar content, although some blue light is present, suggesting at least some star formation is occurring. There is no obvious sign of strong tidal features or recent major merger events, though subtle asymmetries might suggest minor gravitational interactions. It appears to be an isolated galaxy.
