The observed galaxy exhibits a morphology consistent with a spiral galaxy, although the spiral arm structure is not sharply defined. The central bulge appears prominent and moderately sized, contributing significantly to the overall luminosity. A bar-like structure is strongly suggested, bisecting the bulge region. The disk component is visible, but appears relatively smooth and featureless with only hints of spiral arms. The galaxy does not show obvious signs of major mergers, though minor disturbances cannot be ruled out. The overall color profile suggests ongoing star formation. Based on the estimated half-light radius, the galaxy appears to be a fairly typical spiral galaxy.
