The object appears to be a galaxy at a moderate redshift. Morphologically, it displays a structure that is predominantly smooth, though some features or a faint disk-like component may be present. The galaxy exhibits an intermediate roundness, appearing neither perfectly spherical nor highly elongated. There is an indication of possible minor disturbance, but no strong signs of ongoing major merger activity, even though some evidence suggests it could be merging. Its estimated size is about 9 kpc. Based on the color indices, there is evidence of active star formation occurring in the galaxy.
