The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits a near-circular morphology, with a high degree of roundness and a lack of discernible spiral arm structures. The color profile suggests a dominant population of older stars, indicated by the reddish hue concentrated in the central bulge. There is a subtle color gradient moving outward from the core, hinting at a modest amount of ongoing or recent star formation in the outer regions of the galaxy. There is evidence of a possible interaction or minor disturbance with a smaller, fainter companion galaxy nearby. Overall, the galaxy appears to be an elliptical galaxy.
