The galaxy presents a clear spiral structure, with multiple arms extending from a central region. These arms display a tightly wound morphology. The dominant color of the spiral arms is blue, suggestive of ongoing star formation. A prominent bulge appears at the center of the galaxy. There is no apparent bar-like structure traversing the bulge. The galaxy appears relatively isolated with no signs of major merging activity, though minor disturbances cannot be ruled out. The arms also indicate a high spiral arm count, with many tightly wound features. The bulge may be small compared to the overall size of the galaxy. The nucleus appears bright, surrounded by a diffuse glow. The galaxy's disk is oriented face-on relative to our line of sight.
