The galaxy presents as a relatively small, disk-shaped object with a noticeable ring structure. The central region appears brighter and more compact, exhibiting a bluer hue, potentially indicating a higher concentration of younger, hotter stars or active galactic nuclei activity. The ring structure surrounding the core displays a reddish tint, which may be attributed to the presence of older stellar populations and dust. Faint, diffuse extensions are observed outside of the ring, hinting at a larger, less dense halo. The overall morphology suggests a relatively undisturbed system, although there is some evidence of potential minor tidal interactions or internal disturbances contributing to its unique ring structure. The smooth appearance of the main body indicates a potentially earlier-type spiral or lenticular galaxy, but the outer extensions make classification somewhat ambiguous.
