The galaxy presents a largely smooth, rounded morphology, suggestive of an elliptical type or a spiral galaxy viewed face-on with a dominant bulge. Its light profile appears concentrated, with a bright central region that decreases in intensity moving outwards. The galaxy exhibits a reddish-yellow hue, implying an older stellar population with relatively little ongoing star formation. There is an object nearby that could be a star, another galaxy, or even a star cluster within the galaxy. Additionally, the galaxy could be merging with a nearby object based on the asymmetrical shape of its morphology.
