The galaxy appears to be an elliptical type, characterized by its generally smooth and featureless morphology. Its overall shape is roughly spherical. A concentration of light is observed toward the center, indicative of a bulge. The galaxy exhibits a yellowish-orange hue in the central region, potentially due to a population of older stars. The light intensity gradually decreases moving outward from the central bulge toward the edges of the galaxy. There is no apparent disk structure or spiral arm features. Minor asymmetry may be present in the outer regions. There is no evidence of any ongoing major merger events.
