The galaxy exhibits a disk-like morphology, appearing somewhat elongated. It presents with a moderately bright central bulge exhibiting a yellow-white hue, indicative of an older stellar population. The disk component appears fainter and bluer than the central bulge, suggestive of ongoing star formation. The disk also seems slightly warped on one side.

Based on the overall structure, this galaxy could be classified as a spiral galaxy seen at a relatively high inclination, but the resolution of the image makes precise classification difficult. There is no clear evidence of a prominent bar structure. There are no signs of strong tidal interactions or mergers. It also appears to be a single relatively undisturbed system.
