The galaxy appears to be a relatively smooth, elliptical or lenticular system. It exhibits a centrally concentrated luminosity profile, with a gradual decrease in brightness outward from the core. The overall color is somewhat red, suggesting an older stellar population and reduced ongoing star formation. There is no distinct spiral arm structure or significant dust lane obscuration visible. The morphology appears mostly undisturbed, with no signs of major mergers or tidal features. A slight asymmetry or minor disturbance could be present in the outer regions, but is not definitively observed.
