The galaxy presents a spiral morphology, with a prominent central bulge appearing bright and yellow, suggesting a population of older, redder stars. The spiral arms are well-defined, but appear somewhat tightly wound around the bulge. They exhibit a blueish tinge, indicative of ongoing star formation. The disk is viewed at an angle, providing a clear view of the spiral structure. There's no obvious bar structure. Indications of a moderate-sized bulge can be observed based on the brightness and spread in the central regions. There appears to be no major merging or tidal disturbances evident. Based on the arm color and estimated size, the galaxy shows evidence of significant star formation activity.
