The galaxy presents as a spiral type, with a disk-like structure oriented somewhat face-on. A prominent central bulge is evident, exhibiting a yellowish hue indicative of an older stellar population. The spiral arms are readily discernible, displaying a relatively tightly wound morphology. The galaxy appears to have two main spiral arms. Some evidence suggest the presence of a bar feature bisecting the bulge, but this is not especially prominent. Star formation appears to be ongoing within the spiral arms. The overall color suggests the presence of both younger, bluer stars and older, redder stars within the galaxy. There are no obvious signs of major disturbances or ongoing merging events, although there may be minor irregularities in the outer regions of the arms.