The galaxy presents as a centrally concentrated, smooth object, exhibiting an elliptical morphology. The luminosity profile appears to be centrally peaked, with a gradual decrease in brightness moving outwards from the core. The dominant color is a yellow-white hue, suggesting an older stellar population. There is no discernible spiral arm structure or dust lane features visible. The galaxy exhibits a high degree of symmetry and roundness. There's no strong evidence of any major ongoing merger events or tidal disturbances affecting its overall form.
