The galaxy appears as a centrally concentrated, relatively smooth object. The light distribution suggests a spheroidal morphology. There is a high degree of central concentration, with light intensity decreasing steadily outward from a bright core, and then dimming more rapidly. The galaxy exhibits an overall round shape, with minimal deviation from circular symmetry. There is subtle color variation across the galaxy, with the central region appearing more yellow-white, transitioning to a slightly bluer hue in the outer regions. There are no readily apparent signs of spiral arms, bars, or significant dust lanes within the galaxy. No signs of tidal disruption or ongoing major merger events are apparent.