This galaxy appears to be an elliptical type, characterized by a smooth, featureless morphology. Its overall shape is somewhat elongated, though it exhibits a predominantly rounded appearance. The light distribution suggests a centrally concentrated structure, with a gradual decrease in brightness towards the outer regions. The core exhibits a yellowish hue, potentially indicating an older stellar population. No distinct spiral arms or prominent dust lanes are visible. There is no obvious indication of active merging activity or major disturbances in the galaxy's structure, although subtle disturbances cannot be ruled out based on the available image resolution.
