The galaxy presents as a relatively smooth, centrally concentrated object. Its morphology is elliptical or possibly lenticular, exhibiting high degree of central bulge prominence. The luminosity appears to gradually decrease from the core outwards, which has a bright, well-defined central core. A hint of spiral arm structure is visible with only some subtle features that emerge from the central bulge. A very small perturbation may be visible but it is very minor, so it seems to not be interacting with any other objects. The object's color exhibits a blueish white tinge, suggesting active star formation although the galaxy itself is mostly red, showing it to be mostly older stars.
