The galaxy presents as a face-on spiral, exhibiting a well-defined disk structure. Two dominant spiral arms emanate from the galactic center, tracing a grand design pattern. These arms are moderately wound and exhibit some patchiness in their light distribution, suggesting regions of active star formation interspersed with areas of older stellar populations. The central bulge appears relatively small in comparison to the overall disk size and has a weak bar. The galaxy's colour suggests a mix of stellar populations. There are no apparent signs of any major tidal disturbances or ongoing major merging events. The spiral arms have a medium winding, with loose regions as well. 