The galaxy presents a generally smooth and rounded morphology. Its light profile suggests a concentrated central bulge with a gradual decrease in luminosity towards the outer regions. There is faint evidence of a subtle disk-like structure, though the overall appearance is dominated by the bulge component. The color profile of the galaxy indicates a reddish hue. The galaxy appears isolated, with no immediate signs of major mergers or significant tidal disturbances. The galaxy is considered to be a luminous object.
