The galaxy presents as a centrally concentrated, relatively smooth structure. The core exhibits a bright, intense luminosity, suggestive of a high stellar density and possibly an active galactic nucleus. The outer regions fade gradually into the background, with a predominantly elliptical morphology. There is no discernible spiral arm structure or significant dust lane obscuration evident in this image. The overall color appears to be a slightly reddish hue which indicates an older stellar population and relatively low star formation activity. There is little evidence of ongoing mergers or tidal disturbances, the galaxy appears relatively isolated and undisturbed.
