The galaxy presents as a relatively smooth and rounded system, although with some indication of a possible disk-like structure. The primary light emission appears concentrated towards the galaxy's center, which exhibits a brighter, more intense glow. We can see it is an elliptical galaxy that is at a redshift of around 0.09.

The central region may harbor an older stellar population. Further observations are needed to confirm these details and determine the specific morphological classification of the galaxy.
