The galaxy presents as a relatively smooth, elliptical morphology with a high degree of central concentration. There appears to be minimal evidence of spiral arms or other disk-like structures. The light profile suggests a fairly regular shape, with a slight ellipticity that deviates from a perfect circle. There are no visible signs of ongoing major mergers or significant tidal disturbances within the galaxy's structure, it appears to be isolated. Color gradients suggest older stellar populations, but there may be younger stars closer to the center.