The galaxy presents a largely smooth, elliptical morphology. There is a slight ellipticity to the shape, tending towards round but not perfectly spherical. The central region appears brighter and more concentrated, showing a yellowish hue, likely indicating an older stellar population. The outer regions fade gradually into the background, with a subtle reddish tint surrounding the central core. There is no evidence of strong spiral arm structures or significant dust lanes. There do not appear to be any signs of major merging events or tidal disturbances affecting its overall structure, although there are signs of minor disturbances. The galaxy appears to be a relatively quiescent system, exhibiting a low rate of star formation.
