The galaxy presents as a relatively smooth, elliptical-like structure. It appears more elongated than perfectly circular, exhibiting an in-between rounded shape. The galaxy displays a central concentration of light, suggestive of a bulge component. This central region emits primarily yellow-white light, possibly indicating an older stellar population within the bulge. Surrounding this central region, a fainter and more diffuse halo or disk component is visible. This outer region exhibits a slightly bluer hue compared to the central bulge, potentially indicating the presence of some ongoing star formation. Overall, the galaxy appears relatively undisturbed, showing minimal signs of major mergers or significant tidal interactions. There is subtle irregularity to the outermost regions, though, perhaps suggestive of minor interactions.
