The galaxy presents as a relatively smooth, elliptical-like object. The central region exhibits a higher concentration of light, appearing yellowish, suggesting an older stellar population is dominant there. The outer regions show a gradual decrease in luminosity with a faint, diffuse blue-ish halo. This suggests a lower level of current star formation activity, with some remaining younger stars on the edges. The overall structure appears undisturbed, with no obvious signs of major mergers or tidal interactions. There might be some small disturbances. The galaxy appears almost perfectly circular.
