The galaxy presents as a spiral type, characterized by a prominent, luminous central bulge. The spiral arms are relatively tightly wound around the bulge, displaying a noticeable but not overwhelming star formation activity. The overall color of the galaxy suggests a mix of stellar populations, with bluer regions in the arms indicating younger stars and redder hues in the bulge potentially associated with an older population. There is a faint bar-like structure visible, bisecting the bulge. The disk appears relatively undisturbed, without any major signs of recent mergers or interactions. The galaxy exhibits a moderate inclination relative to our line of sight, allowing for a partial view of its spiral structure.
