The galaxy presents a centrally concentrated morphology, appearing predominantly smooth in its light distribution. A notable tidal tail extends from the main galactic body. The main body exhibits a slightly elongated shape, with the tidal tail extending outwards. In terms of color, the central region appears relatively redder, with the outer regions of the tidal tail appearing bluer. This may suggest differing stellar populations within the galaxy, with a higher concentration of older, redder stars in the core and younger, bluer stars in the tail. There also appears to be some disruption happening with the main galaxy body that may be indicative of a recent merger event. 
