The galaxy appears to be an elliptical galaxy, characterized by a smooth, concentrated central region. The light profile suggests a relatively high degree of symmetry, with a gradual decrease in luminosity from the core outward. The color of the galaxy is generally redder, indicative of an older stellar population. There are no prominent spiral arms or dust lanes visible. Its overall shape is more rounded, with only a slight deviation from a perfect sphere. There is no evidence of any major merging activity or significant tidal disturbances.
