The galaxy presents as a relatively smooth, centrally concentrated object with a roughly elliptical morphology. There is little evidence of distinct spiral arm structure or prominent features. The central region appears brighter and exhibits a yellowish-orange hue, potentially indicating an older stellar population. The outer regions fade into a dimmer, slightly bluer color, suggesting the presence of some younger stars. The overall roundness suggests it is likely an elliptical galaxy, with a slight deviation toward an intermediate shape. There is no obvious visual indication of any major ongoing merger activity or significant tidal disturbances.
