The galaxy presents a disk-like morphology with a prominent spiral structure. Multiple spiral arms appear to emanate from a central bulge region. The arms display a patchy distribution of luminosity, indicative of varying stellar densities and potential star-forming regions. A bar structure may be weakly present across the central region. The bulge appears moderately sized. There is no visual evidence of significant tidal disturbances or ongoing major mergers, although minor interactions cannot be ruled out based on the visual data alone. The galaxy appears to be actively forming stars.
