The galaxy appears to be elliptical in shape, with a smooth, largely featureless light distribution. The galaxy exhibits a bright, concentrated central region that fades gradually towards its outer edges. The overall color appears to be skewed towards the redder end of the spectrum with minimal blue light, suggesting an older stellar population and low star formation rate. There are no apparent spiral arms, dust lanes, or signs of ongoing mergers or tidal disturbances. The galaxy's profile is generally uniform, lacking any distinct substructures or asymmetries. The round shape and lack of irregular features suggest a relaxed, dynamically stable system.
