The galaxy presents an elliptical morphology, displaying a centrally concentrated, smooth light distribution with a gradual decline in surface brightness towards its outer regions. The galaxy's color profile appears to be relatively uniform, trending slightly redder toward the core. No distinct features such as spiral arms or a prominent dust lane are discernible within the resolution limits of the image. There is no visible evidence of strong tidal interactions or morphological disturbances, suggesting a relatively relaxed and undisturbed system, and no obvious merging activity. The galaxy appears to be in a relatively isolated environment. 
