The galaxy presents as a slightly elongated, relatively smooth structure. The central region exhibits a yellowish-white color, potentially indicating a population of older stars. A faint, diffuse outer halo extends from this core, displaying a bluer hue which may signify ongoing or recent star formation. There is a bright, blue region that lies close to the galaxy. Overall, there appears to be some asymmetry in the galaxy's structure, possibly suggesting past interactions or internal dynamical processes influencing its morphology.
