The galaxy presents as a slightly elongated, elliptical-like structure with a smooth, featureless appearance. The light distribution appears relatively uniform across the galaxy's body with no strong central concentration. There is some indication that it is not perfectly rounded, trending toward a cigar-shaped morphology. The galaxy appears isolated, with no obvious signs of major mergers or significant tidal disturbances, although minor disturbances cannot be completely ruled out based on the image alone. The color index suggests that the galaxy is composed of a relatively old stellar population, with low star-formation rate and weak blue emission, typical of galaxies with little ongoing star formation. The galaxy shows a slight tendency to be red. Overall, the morphology indicates a mature galaxy that is evolving passively.