The galaxy presents as an elliptical morphology, appearing largely smooth and featureless. There is a concentrated central bulge with a yellow-orange hue, suggesting a population of older stars. The isophotes are generally round, showing a slight deviation toward an intermediate shape rather than a highly elongated one.

There are no apparent signs of spiral arms or a distinct disk structure. Faint extensions are observed around the central region. Overall, the galaxy appears relatively undisturbed, with no obvious indications of recent or ongoing major merger events. The color suggests minimal ongoing star formation activity.
