The galaxy presents as a spiral type, exhibiting well-defined spiral arms that originate from a central region. There appears to be a bar-like structure running through the galaxy's nucleus. The tightness of the winding of the spiral arms varies, appearing moderately wound with some arms appearing more tightly wound than others. 

The central bulge seems relatively small in comparison to the overall disk size. The colors across the galaxy vary, with the central bulge exhibiting a yellowish hue, while the spiral arms display a bluer tint, potentially indicating the presence of younger stellar populations within them.

There are visible irregularities within the spiral arms, suggesting possible minor gravitational interactions or ongoing star formation regions. The overall structure does not indicate a recent major merger, but a possible minor disturbance cannot be ruled out. The spiral arms are relatively well-defined, with at least two or three distinct arms visible.
