The galaxy exhibits a roughly elliptical morphology, appearing somewhat compact. The central region displays a high surface brightness, suggesting a concentrated distribution of stars or an active galactic nucleus. Fainter, diffuse structures are visible extending outwards, these appear asymmetric. There is a hint of distortion in the galaxy's overall shape, possibly due to gravitational interaction or tidal forces. Color gradients across the galaxy suggest variations in stellar populations or dust content. The central core appears bluer compared to the outer regions. The image hints at ongoing or recent disturbances to the structure of the galaxy.
