The galaxy appears as a centrally concentrated spheroid, displaying a relatively smooth, featureless morphology. The core exhibits a yellowish hue, suggesting a population of older stars. There is a subtle color gradient extending outwards from the center, becoming slightly redder towards the periphery. The galaxy lacks any discernible spiral arms or prominent dust lanes. The overall light distribution indicates minimal ongoing star formation. The galaxy's shape is elliptical and nearly round. There is no visual evidence of any major merger activity or significant tidal disturbances, although a very subtle asymmetry might indicate a minor interaction in the past.
