The galaxy presents as a spiral type, with a central bulge region that appears relatively smooth and concentrated. Faint spiral arms extend outwards from this central region. The arms appear somewhat flocculent in nature, with regions of enhanced star formation indicated by localized bluer concentrations. Dust lanes are faintly visible within the spiral arms. The overall ellipticity of the galaxy suggests it is observed at a slight inclination to our line of sight. There is no obvious evidence of a strong bar structure. The galaxy has an estimated size of approximately 5 kpc. The galaxy exhibits a moderate level of star formation activity.
