The galaxy presents as a relatively smooth, disk-shaped object with a pronounced central bulge. The bulge exhibits a yellowish hue, suggesting a population of older stars. Moving outward from the bulge, the disk shows a gradual transition to bluer colors. This suggests ongoing star formation within the disk, with regions of younger, hotter stars contributing to the blue light. The galaxy is elongated, showing evidence of spiral arm structure, though the arms appear tightly wound and somewhat indistinct. Overall, the galaxy exhibits a moderate inclination relative to our line of sight. There is no obvious evidence of a major ongoing merger, but there appears to be some slight distortion in the galaxy's morphology.
