The galaxy presents a relatively smooth, elliptical morphology. It exhibits a bright, concentrated core which suggests a high stellar density. The light from the core is consistent with an older stellar population. Extending outward from the core, the light gradually diminishes. There is a very slight elongation, with a minor axis approximately 0.9 times the length of the major axis. The overall color of the galaxy appears red-shifted. There are no obvious spiral arm structures or dust lanes visible, supporting its classification as an elliptical galaxy with Sersic index ~3. The galaxy’s size is consistent with that of a typical intermediate galaxy with a radius of around 7 kpc. There is little evidence of on-going star formation.
