The galaxy presents a centrally concentrated light profile, appearing as a diffuse, elliptical object. The core region exhibits a yellowish-white hue, suggesting a population of older stars. Moving outwards from the core, the color shifts towards a bluer tint, possibly indicative of younger stars. Faint, asymmetrical extensions or disturbances are subtly visible, suggesting possible tidal interactions or past minor merger events. The galaxy's overall morphology appears to be smooth, with no clearly defined spiral arms or strong dust lanes discernible. The overall shape is somewhat rounded, exhibiting an intermediate ellipticity. There are no indications of major, ongoing mergers.
