The galaxy presents as a relatively compact, somewhat elliptical structure. It appears to be a smooth galaxy, lacking prominent spiral arms or a central bar. The galaxy exhibits a yellowish-orange hue, suggestive of an older stellar population. There is a very slight elongation observed; it is not perfectly spherical. There is little evidence of significant dust lanes or active star formation regions from the color of the galaxy. The galaxy appears undisturbed, with no obvious signs of recent major mergers or tidal interactions.
