The galaxy presents as a centrally concentrated, elliptical-like structure with a smooth light profile. The core exhibits a bright, yellowish-white hue, suggesting a population of older stars. The light becomes slightly redder and dimmer with distance from the center. It has an estimated size of roughly 8.5 kpc based on its Petrosian half-light radius. There appear to be no distinct spiral arms or prominent dust lanes visible. There is no clear evidence of a major merger event, although there may be a minor tidal disturbance or an interacting companion. Overall the galaxy appears to be undergoing minimal star formation.
