The galaxy presents as a moderately sized, somewhat irregular object. The central region exhibits high luminosity, appearing nearly unresolved and indicative of a significant concentration of stars and/or an active galactic nucleus. A faint, diffuse halo surrounds this bright core, extending asymmetrically. There is evidence of a possible tidal tail or a region experiencing gravitational disturbance on one side of the galaxy, indicating possible interaction with another galaxy or a recent merger event. Overall, the galaxy appears to be in a state of dynamic activity, not exhibiting a smooth, well-defined structure.
