The galaxy presents as a slightly elongated, distorted structure with a moderate degree of disturbance. It is characterized by a bright central region, suggesting a concentration of stars or potentially an active galactic nucleus. The colour distribution shows a gradient, with the central region appearing bluer and the outer regions exhibiting a shift towards redder hues. This may indicate differing stellar populations or dust content across the galaxy. The general shape is somewhat amorphous, hinting at possible gravitational interactions or past merger events. Faint extensions are discernible, further supporting the likelihood of tidal disturbances. There is not a distinctive spiral arm structure.
