The galaxy presents as a spiral type, exhibiting a disk structure. The spiral arms are clearly discernible and appear to be well-defined, wrapping around the central bulge. The bulge itself appears relatively small in comparison to the disk. The galaxy's color profile suggests a mix of stellar populations, with a yellower central region indicating older, redder stars, and bluer hues in the spiral arms suggestive of ongoing star formation. There is no apparent bar structure. The overall morphology seems relatively undisturbed, with no major signs of interaction or recent mergers. The orientation of the galaxy is nearly face-on.
