The observed galaxy presents as a relatively small, elliptical morphology. It exhibits a bright central bulge, which appears roughly circular, with a high surface brightness suggesting a concentrated stellar population. Surrounding the bulge is a flattened disk, viewed at a high inclination angle. This disk shows subtle color variations, possibly indicating differences in stellar populations or dust content across the disk. The overall color appears slightly blue, hinting at the presence of younger, hotter stars within the galaxy. There is a possibility of minor morphological disturbance, visible as slight asymmetry in the outer regions of the disk.
