The galaxy presents as a largely smooth, centrally concentrated object with a generally elliptical morphology. There is a pronounced, bright core that fades outwards to a less luminous, diffuse halo or bulge. No distinct spiral arm structures or bar features are discernible. The overall color appears to be somewhat redder, indicating a potentially older stellar population with suppressed current star formation. There is a lack of any obvious signs of tidal disturbances or ongoing mergers, suggesting a relatively settled state. The galaxy appears relatively isolated within its local environment based on the absence of nearby interacting galaxies. 
