The galaxy appears to be a relatively smooth, elliptical galaxy with a high degree of central concentration. It exhibits a generally round morphology, although there is a slight elongation present. It is estimated to be a galaxy with substantial mass, located at a redshift of approximately 0.113.

The galaxy appears to be undergoing a merger event, as indicated by apparent tidal features or distortions in its overall shape. This suggests it is not a relaxed system, and gravitational interactions are likely influencing its structure. Star formation activity appears to be subdued, with a low star formation rate, and a relatively low specific star formation rate. This is consistent with its overall smooth morphology.
