The galaxy appears to be a spiral galaxy, exhibiting a distinct but compact disk structure. The spiral arms are tightly wound around a moderately sized bulge, which dominates the central region.

There is likely star formation occurring within the spiral arms, indicated by subtle bluer regions contrasting with the overall yellow-red hue indicative of older stellar populations. There is little evidence of active galactic nuclei activity in the core. The galaxy doesn't seem to show any signs of significant interaction or recent merging events.
