The galaxy appears to be an elliptical galaxy with a smooth, relatively featureless morphology. It presents a bright, concentrated central bulge, surrounded by a more diffuse halo. There is no apparent spiral arm structure. The galaxy is generally round in shape. Based on the color gradient, the galaxy likely has a population of older stars. There is little evidence of ongoing star formation within the galaxy. There are no signs of major mergers or tidal disturbances. The galaxy appears to be relatively isolated, with no other galaxies visibly interacting with it.
