The galaxy presents as a concentrated spheroid of light, approximately 7 kiloparsecs in radius. The central region is a dominant yellow-white hue, suggesting an older stellar population. The light fades smoothly from the center to the outer edges. The galaxy exhibits a generally smooth texture, lacking any prominent spiral arms or distinct dust lanes. There is a slight deviation from perfect roundness, leaning towards a slightly elliptical shape. There is no visual evidence of any major ongoing merger events, although a faint disturbance might be present in its outer halo. It seems the galaxy is not actively forming new stars, presenting mostly older populations of stars. Overall, the galaxy appears to be a relatively massive, quiescent elliptical galaxy with a smooth morphology.
