The galaxy presents a somewhat amorphous morphology. While it exhibits a central bulge-like structure with high luminosity, there is also the presence of a disk-like component. The disk does not exhibit well-defined spiral arms. The galactic disk seems to have noticeable disturbances. There may be potential signs of merging with another galaxy in the form of tidal tails or distortions. Star formation is present but not very intense. The light appears to originate from an older stellar population, suggesting this galaxy may have an established age.
