The galaxy presents a generally smooth morphology with a slightly elliptical shape. There is a concentration of light toward the center, suggesting a bulge component, which fades gradually outward into a more diffuse halo or disk. Subtle hints of faint, extended structures possibly indicating spiral arms or tidal features can be observed. The color appears bluish-white, potentially indicative of a population of relatively young, hot stars. There is a slight indication of ongoing or recent star formation, and the system may be in the process of undergoing or recovering from a minor merger event due to the irregular outer structures. The overall structure is reasonably well-defined, however, the arms are disturbed.