The galaxy presents as a spiral type, exhibiting a well-defined disk structure. The orientation of the galaxy is close to edge-on. Two prominent spiral arms are observed, appearing relatively loose in their winding, and tracing outwards from the central bulge. 

The central bulge appears moderately sized, exhibiting a yellowish hue indicating an older stellar population. The disk shows signs of star formation with regions of bluer color. The galaxy does not exhibit any signs of major merging events, although minor disturbances in the disk might suggest past or ongoing interactions. A weak bar structure appears to traverse the central region of the galaxy.
