The galaxy appears to be an elliptical galaxy exhibiting a smooth, relatively featureless morphology. It is characterized by a centrally concentrated luminosity profile, with a gradual decrease in brightness towards the outer regions. The galaxy presents an overall rounded shape. There are no prominent spiral arms, bar structures, or dust lanes visible. A slight color gradient is observed, with a subtle yellow hue in the central region transitioning to a slightly redder color in the outer parts. This suggests a population of older stars in the core and a comparatively younger stellar population in the outskirts, though the color difference is not pronounced. There is no evidence of ongoing major mergers or significant tidal disturbances. A subtle asymmetry might be present, indicating a potential minor interaction or recent accretion event, but this is not definitively clear from the available imagery.
