The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits a distinct elliptical morphology, appearing highly rounded in shape, and seen nearly edge-on. There is a noticeable color gradient from the center outwards. The core region exhibits a bright, yellowish-white hue, suggesting a population of older stars. Proceeding outwards, the color shifts to a more reddish tint, possibly indicating the presence of dust obscuration or a different stellar population distribution. There is no prominent evidence of spiral arms or any significant disturbance in its structure, indicating this is likely an early type galaxy. There is no indication of a major merging event or significant tidal features.
