The galaxy presents a primarily smooth morphology, exhibiting a concentrated central bulge. There is some disruption around the central bulge, but the galaxy appears mostly smooth. The overall shape deviates slightly from being perfectly round, leaning towards an intermediate, oval-like structure.  Hints of tidal tails or other merger signatures might exist, indicating recent or ongoing gravitational interactions. Color gradients within the galaxy are visible, with the central regions appearing more yellow/gold suggesting an older stellar population. Some bluer components are visible, possibly indicating regions of younger stars.
