The galaxy presents as a centrally concentrated system. Its morphology appears predominantly smooth with a subtle, diffuse halo. The central region exhibits a yellowish-orange hue, suggestive of an older stellar population. A faint, greenish tinge permeates the outer regions. There is a slight asymmetry to the galaxy's overall shape, possibly indicative of a minor gravitational interaction or internal dynamics. The color gradient from the center to the edges indicates potential differences in stellar populations or dust content across the galaxy. There is no apparent sign of a prominent disk or spiral structure. The galaxy appears relatively isolated.
