The galaxy exhibits a clear disk structure with a moderately inclined orientation relative to our line of sight. Evidence of spiral arms is present, though they appear somewhat flocculent and not tightly wound. There's a central bulge, that appears to be comparatively smaller. Star formation seems to be ongoing within the galaxy, especially in the arms, based on the presence of brighter knots of blue light, potentially indicating HII regions. The overall color of the galaxy suggests a mix of stellar populations, with a relatively blue hue indicative of recent star formation. The shape is elongated, with one axis considerably longer than the other.
