The galaxy presents as a spiral type. Its structure reveals a prominent central bulge, which appears yellowish-white.  There is a disk component, though not perfectly smooth, with hints of spiral arm structure. These arms display mottled regions which suggest active star formation areas, exhibiting a bluer hue than the central bulge. Indications of a possible minor interaction or disturbance are observable in the morphology of the spiral arms. The galaxy is not seen perfectly edge-on, but has a small amount of tilt to the disc. Some possible minor merging or tidal features could be visible.
