The galaxy presents as a spiral type, exhibiting a disk-like morphology with a central bulge. The spiral arms are prominent but somewhat flocculent and loosely wound. There is evidence of active star formation within the arms, indicated by the patchy distribution of bluer light, contrasting with the yellowish hue of the central bulge, which suggests an older stellar population. A bar structure seems to be present, based on a slightly elongated brightening in the center. The galaxy is not perfectly face-on; there may be a slight tilt relative to our line of sight. Overall the galaxy appears relatively isolated, with no obvious signs of major tidal disruption or interaction with other galaxies, although there could be faint evidence of minor disturbances in the outer regions.
