The galaxy appears to be an elliptical galaxy, exhibiting a smooth and mostly featureless morphology. The light distribution is concentrated towards the center, forming a bright, somewhat diffuse core. There is a radial gradient in color, with the core displaying a yellowish-orange hue, potentially indicating an older stellar population. The outer regions of the galaxy exhibit a bluer tint, which may suggest more recent, yet minimal, star formation activity, or a population of younger stars in the periphery. The shape of the galaxy is generally round with little to no observed distortions or asymmetries. No prominent spiral arms, bars, or dust lanes are discernible. The overall impression is that of a relatively evolved, quiescent system. There is no indication of major ongoing mergers or significant tidal disturbances, though the possibility of a minor disturbance cannot be completely ruled out.
