The galaxy presents a largely smooth, elliptical morphology with a concentrated central bulge. It exhibits a yellowish-orange hue, suggestive of an older stellar population with lower levels of recent star formation. There is very little evidence of spiral arms or significant dust lanes within the galaxy. The galaxy appears mostly undisturbed, without prominent tidal features or signs of a recent major merger. Its overall round shape indicates a relatively low degree of intrinsic flattening.
