The galaxy appears as a centrally concentrated object with a smooth, elliptical morphology. It presents a bright, relatively uniform core region that gradually fades outward into a less luminous halo. There is little evidence of distinct spiral arms or prominent features indicative of ongoing star formation. The overall color is slightly yellowish, suggesting an older stellar population with fewer hot, young stars. The galaxy appears undisturbed, lacking any obvious signs of tidal tails or distortions that would suggest a recent merger event.
