The galaxy presents a smooth, elliptical morphology with a concentrated central bulge. There is a distinct lack of resolved spiral arms or dust lanes, suggesting a relatively low rate of current star formation. The galaxy exhibits a fairly uniform color gradient, transitioning from a yellowish core to a slightly bluer halo. The light distribution appears relatively symmetrical, hinting at a dynamically relaxed system. There are no obvious signs of tidal disturbances or ongoing mergers. Overall, the galaxy appears to be a well-formed, early-type system.
