The galaxy presents as a moderately bright, elliptical-like structure. Its core region exhibits a pronounced yellowish-orange hue, suggestive of an older stellar population. The light appears relatively smooth and concentrated towards the center. Fainter, diffuse light extends outward from the central region, fading into the background. There is an apparent lack of distinct spiral arms or significant dust lanes, further supporting its classification as an elliptical galaxy. There are some apparent minor disturbances in the shape of the galaxt. The galaxy appears isolated, without any obvious signs of interaction with neighboring galaxies.
