The galaxy presents as a moderately bright, elliptical-like object. It exhibits a smooth, centrally concentrated luminosity profile with a gradual decline in brightness towards its outer regions. The core appears yellowish, suggesting an older stellar population. The outer regions exhibit a faint bluer tint, potentially indicating the presence of some younger stars, or a low level of ongoing star formation. There is no clear evidence of spiral arms or a defined disk structure. The overall morphology suggests a galaxy that is relatively relaxed, with no prominent signs of recent major mergers or significant disturbances, although very faint tidal features are possible.
