The galaxy presents as a spiral structure with a notable central bulge. The spiral arms are well-defined, exhibiting a somewhat flocculent nature. These arms are characterized by regions of heightened luminosity, suggestive of active star formation. The winding of the arms appears to be of a medium tightness. A subtle bar-like structure is potentially present across the central bulge, though it doesn't seem to be particularly prominent. The galaxy does not show any strong signs of major interaction or merging events with other galaxies, although there is some minor apparent asymmetry. Overall, the galaxy appears relatively undisturbed.
