The galaxy exhibits a relatively smooth, elliptical morphology, lacking prominent spiral arms or a distinct central bar structure. The central region appears brighter and more concentrated in luminosity than the outer regions. A faint blue hue dominates the galaxy's color profile, suggesting the presence of a younger stellar population or ongoing star formation activity. The galaxy appears to have a slight disturbance in its structure, perhaps indicating minor gravitational interactions. Overall, the galaxy displays characteristics consistent with an elliptical or lenticular galaxy type, with a small possibility of a recent or ongoing merger.
