The galaxy presents as a spiral type, observed at a moderate inclination, though not precisely edge-on. A disk component is clearly visible. The spiral arms are evident and moderately defined. While there is a central bulge, it appears relatively small compared to the overall galactic disk. The disk exhibits a patchy distribution of star-forming regions, indicated by the variations in color and luminosity across the disk. There is no significant bar structure that is immediately visible. There does not appear to be any major ongoing merger activity or tidal disruption to the main galactic structure. The galaxy appears to be relatively undisturbed.
