The galaxy presents as a spiral type, with an inclination angled towards the observer, though not perfectly face-on. The spiral arms are clearly visible, extending from a central bulge region. The winding of the spiral arms appears to be of medium tightness. Two primary spiral arms are discernible. The central bulge appears moderate in size, exhibiting a yellowish hue which might indicate an older stellar population. The spiral arms display a bluer tint in comparison to the central bulge, which would be consistent with ongoing star formation. There is no evidence of major mergers, but the shape of the galaxy is not perfectly symmetrical, which could indicate a minor interaction or disturbance. No strong bar feature is evident, though the central region has some elongation suggesting a weak bar presence cannot be ruled out. The estimated size indicates it is a reasonably large galaxy.
