The galaxy presents a discernible spiral structure, although moderately compact. Arms are apparent but not sharply defined, exhibiting a somewhat flocculent morphology. The central bulge region appears prominent and exhibits a yellowish hue, indicative of an older stellar population. A subtle bar structure seems present within the central region. The outer disk shows hints of blue, suggestive of some ongoing star formation. There does not appear to be evidence of major tidal disturbances or significant ongoing mergers. Overall, the galaxy appears to be a relatively normal spiral galaxy with moderate star formation.
