The galaxy presents as a face-on spiral with a prominent, though not dominant, central bulge. The spiral arms are well-defined and exhibit a loosely wound structure. Two primary spiral arms are clearly visible, extending outwards from the central bulge. The colour distribution suggests ongoing star formation, especially within the spiral arms, as indicated by their bluer hue. The bulge appears yellower, potentially signifying an older stellar population. There is a subtle suggestion of a bar-like structure bisecting the bulge. No obvious signs of major mergers are discernible, though minor tidal disturbances are not ruled out. Overall, this appears to be a relatively undisturbed spiral galaxy undergoing active star formation.
