The galaxy presents as a centrally concentrated, luminous object with a nearly circular morphology. It exhibits a smooth, featureless appearance without prominent spiral arms or a distinct disk structure. The light profile suggests a gradual decline in luminosity from the bright core outwards, indicative of a relatively old stellar population. There is little evidence of recent or ongoing major mergers or tidal disturbances. A weak blue hue suggests the presence of some star formation. The overall color appears relatively red, indicating a dominant population of older stars. The size of the galaxy is average with no apparent distortions.
