The galaxy appears as a relatively compact object, approximately 8 kpc in diameter based on estimated Petrosian radius. Its morphology is primarily smooth, exhibiting a high degree of central concentration with a slight elongation. There is some evidence of a very minor disturbance in the symmetry of the galaxy, but overall, it looks like it is not undergoing any major interactions. Judging by the lack of detailed morphology, such as a disk, it likely has an elliptical shape. Its estimated mass is approximately 10^11 solar masses. It seems to be undergoing some star formation. The galaxy exhibits a continuum spectrum that is stronger towards the redder end of the spectrum, indicating the presence of older stellar populations. 
