The galaxy appears to be a relatively smooth, elliptical type with a high degree of central concentration. The light profile suggests a spheroid shape with a gradual decrease in surface brightness from the core outwards. There is little to no visible evidence of spiral arms or a prominent disk structure. The galaxy exhibits a dominant red color, transitioning towards bluer hues near the center. This color gradient could indicate a population of older stars dominating the outer regions and relatively recent star formation in the central region. There appears to be a lack of significant dust lanes or prominent features associated with ongoing merger activity, with only minor disturbances if any. The overall morphology suggests a galaxy that has likely undergone significant dynamical relaxation.
