The galaxy presents as a relatively smooth, elliptical-like structure. Its core exhibits a concentrated luminosity, gradually fading towards the outer edges. The light distribution appears largely uniform without prominent spiral arms or distinct features. The galaxy's color profile suggests a redder population of stars overall. There are no apparent signs of significant ongoing merger events, although subtle asymmetries might indicate minor tidal disturbances. The morphological characteristics point toward a galaxy that is highly rounded in shape. There are no strong, distinct features beyond the smooth shape and the subtle color gradient across the body of the galaxy.
