The galaxy presents as a singular, relatively smooth object. It exhibits a centrally concentrated light profile, appearing nearly spherical in shape. There is little evidence of spiral arm structures or prominent dust lanes. A gradual colour gradient is observed, transitioning from a more yellow-white core to a slightly fainter, greener outer halo. This colour gradient potentially indicates varying stellar populations within the galaxy, with older, redder stars concentrated toward the centre, and younger, bluer stars more dispersed in the outskirts. Overall, the galaxy exhibits characteristics consistent with an elliptical morphology.
