The galaxy presents as a relatively smooth, elliptical-like structure. Its core exhibits a high degree of luminosity, appearing almost uniformly bright. The galaxy displays a subtle elongation, deviating slightly from a perfectly circular form, with an estimated effective radius of approximately 6 kpc. There's a distinct color gradient within the galaxy; the central region appears more yellow/orange in hue, possibly indicating an older stellar population, while the outer edges suggest a bluer tinge, which may signify more recent star formation activity, although this is less prominent. There is no visual evidence of spiral arms, a prominent disk, or any signs of major ongoing mergers or significant tidal disturbances. A small amount of minor asymmetry or disturbance is not ruled out. The overall morphology is consistent with a relatively evolved system.
