The object presents as a relatively bright galaxy, exhibiting a disk-like morphology. The central region displays a concentrated, luminous core, likely indicating a significant stellar population or active galactic nucleus. The disk itself appears somewhat irregular, with a suggestion of internal structure that may be indicative of spiral arms. There is a subtle color gradient across the disk, shifting from a slightly bluer hue in some regions to redder tones elsewhere. Overall, the galaxy displays moderate levels of disturbance and a potential ongoing minor merger.
