The galaxy presents as a face-on spiral, though the arm structure is somewhat indistinct. The central bulge appears prominent and exhibits a smoother texture compared to the outer regions. Overall it has a disk shape and is of intermediate size for the galaxies in the survey. The color of the bulge is slightly redder, which is indicative of an older stellar population. There are hints of bluer regions in the disk, suggesting ongoing star formation, although it is not a very active star forming galaxy. Some irregularities in the shape suggest a past or ongoing interaction, though no clear merger is visible. The galaxy appears relatively isolated in its environment.
