The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a concentrated central bulge with a yellow-orange hue, suggesting an older stellar population. The galaxy appears moderately compact, lacking prominent spiral arms or significant dust lanes. The overall shape is somewhat elongated, but not dramatically so. There is a lack of distinct features indicating an ongoing major merger event, though minor disturbances may be present. Based on the red color, star formation is likely suppressed.
