The galaxy presents as a relatively smooth and rounded structure, lacking significant disk-like features or spiral arms. Its morphology appears largely spheroidal. There are two distinct regions of higher luminosity, one larger and one smaller, which may indicate either distinct concentrations of stars or a central bulge with a companion. The galaxy exhibits a yellowish-orange hue, possibly indicative of an older stellar population. There is no obvious presence of dust lanes or significant star formation regions within the visible light spectrum of this image. Overall, this object appears consistent with an early-type galaxy.
