The galaxy presents an irregular morphology, appearing as a somewhat diffuse structure. The central region exhibits a higher concentration of light, suggesting a possible galactic nucleus or bulge. A pronounced, asymmetrical extension or tidal tail is visible, curving away from the main body. This tail is characterized by a bluer hue, indicative of younger stellar populations or enhanced star formation. The main body displays a more yellowish-red color, potentially due to older stars or dust obscuration. The overall shape suggests ongoing or recent gravitational interaction, possibly a merger event.
