The galaxy presents a predominantly smooth morphology, suggesting an elliptical or lenticular classification. The light profile appears relatively concentrated toward the center, with a gradual decrease in brightness outwards. There is faint color variation, with a central yellowish-white hue that subtly transitions to a redder and dimmer periphery. No distinct spiral arm structures or dust lanes are visible. The overall appearance indicates a system dominated by an older stellar population. The image hints at a moderate mass and a low ongoing rate of star formation. There is some indication of minor disturbances or tidal features, though these are subtle, potentially indicative of past interactions or minor mergers. The shape is somewhat elliptical.
