The galaxy presents as a single, centrally condensed object with a high degree of radial symmetry. The light distribution appears smooth, lacking any discernible spiral arms or bar structures. The core region is bright, exhibiting a high surface brightness, which fades gradually into the outer regions. The galaxy's morphology suggests an elliptical classification, and it appears to be an early-type galaxy. There is no visual evidence of ongoing major mergers or significant tidal disturbances. The color appears relatively uniform across the galaxy, trending slightly towards the redder end of the spectrum. The overall appearance suggests a relatively old stellar population, with minimal recent star formation.
