The galaxy presents a largely smooth, elliptical morphology. It has a concentrated central region, with a radial decrease in brightness outwards. The galaxy exhibits an overall rounded shape. There is no significant evidence of spiral arms or a prominent disk structure. The color profile appears relatively uniform across the galaxy, lacking the distinct blue regions that would indicate active star formation. There are no obvious signs of tidal disturbances, ongoing mergers, or close companions. The galaxy's structure indicates a relatively quiescent and relaxed stellar population.
