The galaxy presents with a somewhat smooth morphology, but also exhibits a distinct disc-like structure. The central region displays a brighter, more concentrated luminosity, suggesting a possible bulge. The overall shape is generally rounded but has slight deviations indicating it may be somewhere between completely round and slightly elliptical. There appears to be some evidence of minor gravitational disturbance, potentially indicating interactions with smaller galaxies or gas clouds. Overall color balance indicates the presence of star formation.
