The galaxy presents a generally smooth and rounded morphology, with a subtle elongation. The central region displays a high surface brightness, appearing nearly uniform in color, possibly indicating a concentrated stellar population. The light from the galaxy fades gradually toward the outer edges. There is a very slight suggestion of a disk-like structure or faint features, but this is difficult to discern. The galaxy appears to be undisturbed, showing no obvious signs of recent major mergers or tidal interactions. The color profile suggests the presence of stars that are on average older.
