The galaxy appears to be an elliptical galaxy, with a smooth, diffuse light distribution lacking discernible spiral arms or a prominent disk. Its overall shape approximates roundness, with a slight deviation toward an intermediate form. The central region exhibits a concentration of light intensity, suggesting a galactic nucleus. There is no visual evidence of active merging or major disturbances in the galaxy's morphology, although subtle irregularities might be present. Overall star formation activity appears to be relatively low.
