The galaxy presents an elliptical morphology, exhibiting a smooth light distribution with a high degree of central concentration. It appears largely featureless, lacking prominent spiral arms or distinct dust lanes. The core displays a bright, yellowish hue, suggesting a population of older stars. The outer regions are less luminous with the presence of a possible faint disk, showing some blue light and subtle color gradients extending outward. These gradients suggest varying stellar populations, with relatively younger star formations towards the edges. Overall, the galaxy seems to be in a relatively quiescent state, with low star-forming activity. A slight elongation is observable, but the isophotes appear generally regular, indicating a relaxed dynamical state.
