The galaxy presents a generally smooth and centrally concentrated morphology, suggesting a classification toward the elliptical or lenticular types. The light distribution is dominated by a prominent central bulge that appears nearly spheroidal in shape. There is only very slight evidence of any features or disk-like structure. Overall, the galaxy appears relatively undisturbed. The color is biased towards the redder end of the spectrum. Given the color and morphology, the galaxy is likely composed primarily of older stellar populations and exhibits a low rate of star formation. The galaxy seems relatively isolated and is not undergoing any significant merger activity.
