The galaxy presents as a relatively smooth, centrally concentrated object. Its shape is approximately round, exhibiting a slightly elliptical morphology. There is a central, bright core that appears to be composed of older stellar populations, with colors trending toward the redder end of the spectrum. Fainter light extends outwards from the core, forming a diffuse halo. There is possible evidence of an arm-like structure, or a minor disturbance on one side of the object. Overall, the galaxy appears to be relatively isolated, with no signs of ongoing major merger activity.
