The galaxy presents a morphology consistent with a spiral, although the structure appears somewhat disrupted. A central bulge is visible, exhibiting a yellowish-white hue. Fainter, bluer light extends from the main body in what seem to be faint and distorted arms.

There is an indication of merging or recent tidal interaction with another galaxy. The primary galaxy's disk appears warped or asymmetric, showing some evidence of tidal tails or streams of stars and gas extending outward. It appears to be in the process of merging with the galaxy directly above the original one.

The overall color suggests a mix of stellar populations, with older, redder stars concentrated in the bulge and younger, bluer stars populating the arms. The star formation appears to be very slow.
