This galaxy presents as a spiral, although its inclination complicates a complete morphological assessment. The disk appears prominent, with evidence of spiral arm structure, although at this resolution, individual arms are not clearly resolved. The spiral arms appear tightly wound.

A central bulge is noticeable, exhibiting a moderate size relative to the overall disk. Its color suggests an older stellar population compared to the bluer disk. There is no sign of a prominent bar structure.

There is also a suggestion of interactions, as the galaxy is somewhat distorted. There are no obvious tidal tails or other dramatic features, suggesting that any interaction is ongoing, or potentially a minor merger.