The galaxy presents as a somewhat lenticular structure, exhibiting a notable central bulge that appears relatively smooth and concentrated. The outer regions display a faint disk-like component. Color gradients are discernible, with the core appearing more yellow/white, suggesting an older stellar population, while the periphery shows a slightly bluer hue, indicative of younger stars or ongoing star formation. There is an adjacent structure with a slight blue hue to the bottom of the main galaxy, indicating that there may be a tidal arm or dwarf galaxy merging with the larger structure. Overall, the galaxy's morphology indicates a system undergoing evolutionary processes, potentially shaped by past or ongoing interactions.
