The galaxy presents as a fairly smooth, elliptical-like structure. It exhibits a concentrated central bulge that graduates outward to a more diffuse halo. The color profile is dominated by warmer tones, suggesting an older stellar population. There are no prominent spiral arms or dust lanes visible. Overall, the galaxy appears relatively undisturbed, with no obvious signs of ongoing major mergers or tidal interactions. There may be some subtle, minor disturbances but nothing obvious. The galaxy is approximately circular in shape.
