The galaxy appears to be a relatively bright elliptical, exhibiting a smooth, concentrated light profile. The core is the most luminous region, displaying a nearly spherical morphology. There's a gradual decrease in luminosity moving outward from the center, with a faint, extended halo subtly merging with the background sky. No distinct spiral arms or dust lanes are discernible within the limits of the image resolution. There are no signs of recent mergers or major disturbances affecting the galaxy's overall structure. The galaxy's roundness suggests a minimal rotational velocity. The overall color is indicative of an older stellar population, with minimal ongoing star formation activity. The galaxy's estimated size suggests a moderate scale within the observed region.