The galaxy presents as a spiral with a prominent, bright central bulge. The bulge appears yellowish-white in color, suggesting an older stellar population. Fainter, bluer spiral arms extend outwards from the bulge. These arms are somewhat fragmented and show evidence of active star formation, as indicated by the patchy blue regions. The galaxy disk is viewed at a moderate inclination, allowing some of the spiral structure to be seen. There are hints of a bar-like structure within the central region. The galaxy doesn't show any signs of major interaction or merging activity. The overall morphology suggests a galaxy that is relatively undisturbed and undergoing normal star formation processes.
