The galaxy presents as a relatively smooth, centrally concentrated object, appearing largely elliptical in shape. There is a slight elongation, but it is generally rounded. It exhibits a noticeable color gradient, transitioning from a bluer hue in the central region to redder tones in the outer portions. No distinct spiral arms or bars are discernible within the available image resolution. There is no evidence of a major ongoing merger event, although there might be a slight asymmetry in the outskirts suggesting a possible minor interaction or past disturbance. Overall, the galaxy appears to be a fairly mature system with a dominant bulge component, a mass slightly above average, and relatively low star formation.
