The galaxy exhibits a morphology suggestive of ongoing interaction or a recent merger event. The main body appears disturbed, lacking a clear spiral or elliptical structure. There are subtle asymmetries in the light distribution.

A faint tidal tail-like feature extends outwards, indicating gravitational disturbance. There may be two distinct nuclei present, though this requires further investigation.

The color distribution is non-uniform, with regions showing bluer colors indicative of active star formation and redder regions possibly representing older stellar populations. The galaxy appears to be of moderate size relative to other galaxies in the surrounding field.
