The galaxy presents as a spiral, exhibiting a prominent disk structure. A discernible central bulge is evident, with a moderate contribution to the overall light profile. Spiral arms are readily apparent and are wound in a medium to loose fashion. The morphology suggests a bar structure is present within the central region, the bar is not strong. The galaxy shows signs of a possible disturbance or interaction, as evidenced by some asymmetries in the spiral arm structure. The color profile shows a gradient from bluer hues in the outer arms to redder hues in the central bulge. This color gradient likely indicates differing stellar populations, with younger, hotter stars populating the arms and older, cooler stars concentrated in the bulge. Some dust lanes appear to be obscuring regions along the spiral arms.
