The galaxy presents as a relatively smooth, centrally concentrated object. Its overall color is slightly red, which likely indicates an older stellar population with fewer young, massive stars. The primary component appears spheroidal, lacking distinct spiral arm structures or a prominent disk. There may be a very slight asymmetry to the overall shape, though it could be due to lensing. This galaxy likely has a considerable mass and is forming relatively few stars. There also is likely no major merger or significant disruption of the galaxy's structure. Based on the red-shifted color, the galaxy is relatively far from us.
