The galaxy presents as a relatively smooth, centrally concentrated object. It appears to be a single, unified structure with a somewhat elliptical shape, though nearly round. There is no strong evidence of spiral arm structure or a prominent disk; it appears largely spheroidal in nature. Faint extensions can be seen towards the outer regions, though they do not present as features typically seen in actively merging galaxies. The color distribution is fairly uniform, with a concentration of bluer light towards the galaxy's core. This suggests ongoing, albeit possibly moderate, star formation in the central region. The overall appearance suggests a galaxy that has largely completed its merging history and is relatively quiescent.
