The galaxy appears to be a relatively compact elliptical galaxy, possessing a smooth, symmetrical morphology. There is no visible evidence of spiral arms or a prominent disk structure. The light profile suggests a centrally concentrated luminosity, with a gradual decrease in intensity toward the outer regions. The color is predominantly yellowish-orange, which indicates an older stellar population, implying that star formation is likely suppressed. There are no apparent signs of significant dust lanes or recent merger activity. The galaxy displays a high degree of roundness. The overall appearance indicates a galaxy that has undergone significant dynamical relaxation and is likely to be dominated by evolved stars.
