The galaxy presents as a somewhat disturbed system, exhibiting a moderately compact central region. The morphology is primarily smooth, but with some irregularities. The galaxy shape appears somewhat rounded with a slight elongation. There is a hint of a possible tidal feature or minor disturbance, which could suggest a past or ongoing interaction with another galaxy or satellite. The color gradient indicates the central region is slightly more yellow/orange, implying the presence of an older stellar population or dust obscuration. The outer regions have a bluer tint, potentially indicating younger stars. Overall, this galaxy appears to be in an intermediate stage of its evolution, having likely undergone past interactions, and still exhibiting some star formation.
