The galaxy presents a largely smooth morphology. The object exhibits a centrally concentrated luminosity profile with a near-circular appearance on the sky, although the shape appears slightly elongated. A bright, inner region is observed within the galaxy, surrounded by a slightly fainter ring of stars. The central, bright structure may indicate the presence of a supermassive black hole. There is a faint but noticeable asymmetry in the outer regions of the galaxy. Star formation rate indicators suggest relatively low star formation activity within the galaxy. Overall, this galaxy may be a lenticular galaxy.
