The galaxy presents as a relatively face-on spiral with a prominent bulge. The central region exhibits a yellowish hue, indicating a population of older stars. The disk of the galaxy shows some evidence of spiral arm structure, but it appears somewhat flocculent and not sharply defined. Dust lanes are subtle but present in the disk. The outer regions of the galaxy fade in intensity. There is evidence of ongoing star formation within the disk, hinted at by the slightly bluer color in some regions, though this is subtle overall. The galaxy exhibits a moderate amount of rotational symmetry, and the disk is not highly inclined. No strong bar structure is apparent. There is little evidence of active galactic nuclei activity based on color. The galaxy is not undergoing any major merger activity.
