The galaxy presents a predominantly smooth morphology, with a centrally concentrated bulge exhibiting a yellowish-red hue. Surrounding the bulge is a fainter, more diffuse disk component that appears bluish. While generally smooth, there are hints of minor disturbances in the disk structure, possibly indicative of a weak interaction or internal processes. The overall shape appears to be neither perfectly round nor highly elongated, presenting an intermediate aspect. There is some evidence of possible star formation in the blue areas, which tend to be further from the bulge.
