The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge. It exhibits a predominantly yellow hue, indicative of an older stellar population. There are subtle color gradients, with the central region appearing more intensely yellow, potentially suggesting a higher concentration of older, redder stars. The outskirts of the galaxy are less defined, fading into the background, though there is some slight reddening towards the exterior. The shape is generally round. There is no obvious evidence of spiral arms or significant dust lanes; neither are there any prominent features to suggest a recent or ongoing major merger event.
