The galaxy presents as a relatively smooth, elliptical structure with a concentrated central bulge. The color profile indicates a dominance of older stellar populations, evident in the yellowish hue. There is little discernible dust or spiral arm structure. The galaxy appears largely undisturbed, exhibiting no signs of ongoing major mergers or significant tidal distortions. A faint, diffuse halo may be present, though it is difficult to distinguish it from the background sky. Overall, the morphology suggests an evolved galaxy with a quiescent star formation history.
