This galaxy presents a flattened, disk-like structure. The central region appears relatively smooth and amorphous, with a gradual increase in surface brightness toward the core. The outer regions of the galaxy exhibit a bluer hue compared to the core, suggesting the presence of younger stellar populations.

There are hints of possible spiral arm structures, with some slight asymmetries in the light distribution. The galaxy's overall form is somewhat disturbed, showing irregularities. These irregularities may suggest a potential minor interaction or merger event in the past. There also may be a possible tidal tail or bridge that looks like it has lower surface brightness. However, further examination and spectroscopic data would be necessary to confirm these hypotheses and understand the dynamics and composition of the galaxy.
