The galaxy presents as a spiral type, though the spiral arm structure is somewhat indistinct. There is a prominent central bulge that appears quite luminous and exhibits a yellowish hue. Surrounding the bulge is a fainter, more diffuse disk. The disk shows hints of spiral arm structure, but the arms are not sharply defined. Overall, the galaxy exhibits a moderate degree of central concentration. There is no clear indication of a strong bar feature within the disk. The galaxy appears relatively isolated, showing no obvious signs of major merger events or tidal disturbances in this image.
