The galaxy presents a discernible spiral structure, though the arms are somewhat flocculent and not sharply defined. There appears to be a central bulge region that is relatively bright and exhibits a yellowish hue, suggesting an older stellar population. Fainter, bluer regions are observed in the outer disk, likely indicating areas of more recent star formation. The galaxy shows evidence of some gravitational disturbance or interaction, as indicated by the slightly asymmetrical shape of the disk and potential tidal features. Overall, the galaxy appears to be a spiral galaxy undergoing moderate star formation, with a well-established bulge and ongoing activity in the disk.
