The galaxy presents a generally smooth, elliptical morphology, with a subtle central bulge that appears more concentrated and yellow in color, suggestive of an older stellar population. The outer regions of the galaxy are slightly elongated and display a color gradient, transitioning to a slightly bluer hue. This might indicate the presence of younger stars or ongoing star formation within the galactic disk, albeit at a seemingly low rate. There is no discernible evidence of spiral arm structure or significant tidal disturbances indicative of major mergers. The galaxy appears relatively undisturbed, and is somewhere in between round and cigar shaped, which would lead me to believe that it is slightly disk-like.
