The galaxy exhibits a discernible disk-like structure, although its orientation is somewhat oblique relative to our line of sight. Within the disk, spiral arm features are subtly visible, with regions of enhanced brightness suggesting active star formation. The central bulge region appears prominent and relatively smooth in texture. Evident morphological disturbances are visible, indicating a possible interaction or merger event. The galaxy's overall color profile indicates a mix of stellar populations, with bluer regions indicative of younger stars and redder areas suggesting older populations.
