The galaxy exhibits a smooth, elliptical morphology. It appears largely featureless, lacking prominent spiral arms or significant dust lanes. The light distribution is centrally concentrated with a gradual decrease in surface brightness towards the outer regions. The color profile suggests a population of older stars, as indicated by the reddish-yellow hue dominating the galaxy's core and extending outwards. There's no apparent evidence of ongoing major merging activity or significant tidal disturbances; it presents as a relatively undisturbed system. The overall structure indicates a galaxy likely undergoing passive evolution, with reduced or negligible recent star formation.
