The galaxy presents a predominantly smooth morphology, with little discernible substructure. Its overall shape appears largely elliptical, transitioning from a bright, concentrated central bulge to a fainter, more diffuse halo. The central region exhibits a yellowish hue, potentially indicating an older stellar population. The outer regions of the galaxy display a gradual color gradient, transitioning to slightly redder tones. There is no indication of prominent spiral arms or strong tidal disturbances. The galaxy appears relatively isolated, with no obvious signs of ongoing major merger activity or significant interaction with neighboring galaxies.
