The galaxy presents as a spiral, with two prominent arms emanating from the central region. The arms appear somewhat diffuse and exhibit a moderate winding. There is a subtle presence of a stellar bar structure bisecting the galactic nucleus, though it is not particularly pronounced. The central bulge is not prominent, but it is not nonexistent either, though the bulge is small. The galaxy disk dominates its overall appearance, and it's likely not undergoing any significant merging activity, displaying a relatively undisturbed morphology. There are no obvious signs of a recent major merger and it appears to be relatively stable in its current state.
