The galaxy exhibits a prominent, yellowish central bulge, suggestive of an older stellar population. Extending outwards from the bulge are spiral arms, though their structure appears somewhat flocculent and less well-defined. There are hints of some areas of bluer colors mixed with the yellowish/pinkish color of the bulge, indicating some ongoing star formation. The galaxy is at a slight angle to our line of sight, and it is disk dominated. There are possibly two spiral arms present, but this needs to be further assessed. There is a possibility of a very small companion galaxy in the galaxy's halo.
