The galaxy presents as a relatively smooth, elliptical-like structure. There is a concentrated central bulge that appears yellowish, suggesting an older stellar population and diminished star formation activity in the core. The galaxy exhibits a degree of oblateness. The outer regions display a gradual decrease in luminosity, fading into the background sky. There is a hint of a very faint disk. No significant tidal features or distortions are discernible, indicating the absence of recent major mergers or interactions. The galaxy's overall structure is largely undisturbed.