The galaxy presents a generally smooth morphology, appearing elliptical in shape with no discernible spiral arms or significant disk structure. The light distribution is centrally concentrated, with a bright, nearly uniform core that diffuses outwards. There is a gradual decline in surface brightness from the center towards the periphery. The color gradient suggests a population of older stars, with a yellowish hue dominating the central regions, slightly transitioning to redder tones towards the edges, implying that star formation is low. There are no obvious signs of recent or ongoing major merger events or tidal disturbances. The lack of features suggests that this is a relatively evolved system.
