The galaxy presents an elliptical morphology with a smooth, diffused appearance. The central bulge is bright and concentrated, exhibiting a yellowish-white hue, indicating an older stellar population. Moving outward from the core, the luminosity gradually decreases, fading into a less defined halo. There is a slight elongation observed, suggesting it is not perfectly spherical, and it may be of Hubble type E4-E5. No distinct spiral arms or prominent dust lanes are discernible. The color profile is relatively uniform, with no obvious signs of active star formation regions or younger blue stars. The galaxy shows no obvious signs of a major merger, and is likely an early-type galaxy, at a distance of roughly 1 billion light years away.
