The galaxy exhibits a disturbed morphology, with evidence of tidal features and potential interaction with another galaxy or dwarf galaxy. One prominent feature is a bright, slightly elongated central region with a bluish tint, suggesting the presence of a relatively young stellar population and/or active star formation. A faint tidal tail curves away from this central region. The remainder of the galactic structure shows a more diffuse and less structured arrangement of stars and dust. Given these characteristics, the galaxy appears to be undergoing a merging event or experiencing gravitational disruption. The overall color index appears to be relatively blue indicating star formation. 