The galaxy presents as a spiral galaxy with a distinct disk. The disk is moderately inclined relative to our line of sight. The central bulge is prominent and appears moderately sized, with a concentrated bright core. Some asymmetry is visible in the outer disk structure.

There is evidence of ongoing star formation, as suggested by the presence of bluer regions within the spiral arms. Broadly, the colours of the light are weighted towards the green and red, with some blueish areas in the disk.

The galaxy exhibits flocculent spiral arms, implying ongoing, but not particularly organized, star formation. There appears to be a bar-like structure in the center of the galaxy, which could be categorised as moderately strong, likely funnelling gas towards the central region. The overall morphology suggests the galaxy is relatively undisturbed, with no immediately obvious signs of major mergers or significant tidal interactions.
