The galaxy appears to be an elliptical galaxy, with a generally smooth morphology. It exhibits a dominant, concentrated central bulge that transitions into a less distinct halo. The color is predominantly yellow to gold, suggesting a population of older stars. There is no readily apparent spiral structure or significant dust lanes. The galaxy is moderately compact with an estimated effective radius of a few kiloparsecs. It does not display any obvious signs of major merger activity, although a slight asymmetry could indicate a minor interaction in its past.
