The galaxy presents as a slightly elongated object with a prominent, bright central bulge. There appears to be a disk structure, although it is not sharply defined, and the overall shape suggests an intermediate-type spiral or lenticular galaxy.

One arm extends from the disk with some distortion, possibly due to gravitational interaction or past merger events. The color distribution indicates that the central bulge is dominated by older stellar populations, exhibiting a yellowish hue. The disk shows bluer regions, indicative of ongoing star formation, particularly within the arm extending outwards. Dust lanes or regions of obscuration appear subtly within the disk, contributing to its mottled appearance.
