The galaxy presents as a singular, somewhat amorphous structure. The dominant color appears to be a muted yellow-white, with hints of bluer regions intermixed within the diffuse halo. There is a bright yellow concentration, and a second, slightly less bright concentration in the center. It displays a disturbed or complex morphology, possibly indicative of an ongoing or recent interaction. A small percentage of the galaxy is comprised of a reddish component, potentially arising from older stellar populations or dust obscuration. Based on the distribution of light, there is no clear, well-defined spiral arm structure, however there is evidence of disk structure. Evidence suggests the possibility of a minor merger or tidal disturbance. Overall, this galaxy appears to be undergoing significant evolutionary processes.
