The galaxy presents as a centrally concentrated object with a smooth, elliptical morphology. A distinct central bulge is visible, exhibiting a yellow-white hue, suggestive of an older stellar population. The outer regions of the galaxy show a gradual decrease in brightness, with subtle hints of a bluer color, potentially indicating the presence of younger stars or ongoing star formation within the disk. No significant spiral arm structure is discernible. There are no obvious signs of tidal disturbances or interactions with nearby galaxies. The overall impression is that of a relatively quiescent, isolated system. The estimated physical size indicates it is a relatively large galaxy.
