The galaxy presents as a largely featureless, elliptical or spheroidal system. It appears smooth, with a high degree of central concentration of light. There is a distinct lack of spiral arm structures or pronounced dust lanes. The color gradient suggests an older stellar population, trending towards redder hues in the central bulge. There is no evidence of any recent or significant merger events and the system appears relatively undisturbed. It presents a round morphology with a single central concentration of light. The estimated size of the galaxy is several kiloparsecs.