The galaxy presents a generally smooth, elliptical morphology. It exhibits a concentrated, bright central bulge, which appears to dominate the overall light output. Moving outward from the core, the galaxy demonstrates a gradual decline in surface brightness. There is a slight color gradient observable, where the core regions appear more yellow/orange, and the outer regions trend towards a redder hue, suggesting older stellar populations in those areas. There is little evidence of spiral arms or dust lanes. Perturbations in its overall structure are not apparent, indicating it is not currently undergoing a major merger, though a slight tidal tail is possible. The galaxy’s overall structure indicates it is an evolved system with a subdued rate of star formation.