The galaxy presents as a disk galaxy, observed nearly edge-on. There is a prominent central bulge with a somewhat rounded morphology. The disk appears relatively smooth with no clearly resolved spiral arm structure visible at this resolution. The galaxy exhibits a color gradient, with a more yellow/orange hue in the central bulge region, which could indicate an older stellar population or dust obscuration. Fainter, bluer light traces the outer edges of the disk, possibly signifying more recent star formation activity. There is no evidence of major tidal disturbances or ongoing merger activity although subtle minor asymmetry cannot be ruled out.
