The galaxy appears as a centrally concentrated, elliptical-like structure. It exhibits a smooth, largely featureless morphology with a high degree of rotational symmetry. The galaxy's color profile is characterized by a strong red component, suggesting an older stellar population. There are hints of faint, diffuse light extending outwards from the central region, implying a gradual decrease in stellar density with increasing radial distance. No prominent dust lanes, spiral arms, or tidal features are apparent in the image, indicating a lack of recent major merger activity or ongoing star formation.
