The galaxy presents as a primarily smooth, elliptical morphology. There is a concentration of light toward the center of the galaxy, suggesting a bulge. The color profile appears to be redder toward the central bulge, possibly indicating an older stellar population, and bluer around the outskirts of the disk, suggesting some more recent star formation. It shows a slight disk shape, although that is not its main morphology. There is no visual evidence of any strong merging activity or major disturbances, although there is a subtle irregularity in its shape that may suggest a minor disturbance or past interaction. There's little evidence of spiral arm structure. It is somewhat elliptical but trending more toward being in between elliptical and round.
