The galaxy exhibits a disturbed morphology suggestive of a merger event. Two distinct nuclei are not clearly observed, but the light distribution appears asymmetric and irregular. The primary body of the galaxy presents a yellowish-white hue, possibly indicating an older stellar population. A blueish region appears offset from the main galactic body, perhaps indicative of a younger stellar population or regions of active star formation triggered by the interaction. The galaxy is moderately compact with a somewhat diffuse outer structure, lacking a well-defined spiral structure or elliptical profile. Faint tidal features are subtly present, indicating gravitational interaction with another galactic structure.