The galaxy presents a generally smooth, elliptical morphology. It exhibits a bright, concentrated central bulge that appears yellowish-white, possibly indicating an older stellar population. The surrounding disk is less defined but appears bluer in color, suggesting the presence of some younger, hotter stars, though the fraction appears low. There appears to be very little to no presence of spiral arms or a bar structure. Overall, there does not appear to be any current active mergers nor a major disturbance to its general structure. The galaxy is slightly elongated rather than perfectly circular.
