The galaxy presents as a slightly elongated, disk-shaped structure. A bright, concentrated central region is evident, possibly indicative of a bulge. Fainter, extended emission emanates from the central core, appearing more pronounced on one side, and suggests the presence of a disk-like component. There appears to be some signs of disturbance within the galaxy, possibly a slight asymmetry or warp in the disk. A potential arm structure might be present in one area, though it is not well-defined. The color profile suggests a generally older stellar population, although the bluer colors in outer regions indicate younger stars or star formation activity. The general structure suggests that this is possibly a spiral galaxy.
