The galaxy presents as a flattened, disk-like structure, viewed at a slight angle relative to face-on. The central region exhibits a brighter, more concentrated luminosity, suggestive of a bulge. Faint spiral arm structures are possibly present but indistinct. The galaxy's overall color is bluish-white. There is no clear evidence of strong active star formation regions. The overall morphology suggests that the galaxy is an early to intermediate spiral galaxy, where the disk is much brighter than the bulge. The galaxy may have a mass in the range of approximately 5 x 10^9 to 6 x 10^9 solar masses.
