The galaxy presents as a spiral type, with a discernible disk structure and arms. The spiral arms are somewhat tightly wound and extend from a central bulge. The bulge appears prominent and exhibits a yellowish hue. The arms display a bluer color, suggestive of ongoing star formation activity. The overall morphology suggests the galaxy is relatively undisturbed, without major signs of interaction or merging, although there are some minor irregularities in the arm structure that may indicate a past interaction. The galaxy is not viewed edge-on. There is no clear central bar structure. The galaxy is compact.
