The galaxy appears to be a relatively smooth, elliptical-like structure with a concentrated central bulge that exhibits a yellowish hue. There is a slight color gradient visible, with the core being more yellow and the outer regions appearing somewhat bluer, suggesting a difference in stellar populations or dust content between the two regions. No distinct spiral arms or significant dust lanes are apparent; the overall morphology suggests a galaxy dominated by older stellar populations. It exhibits a round overall shape with no visual signs of any merging activity or major disturbances. The galaxy appears to be relatively compact.
