The galaxy appears as a luminous, centrally concentrated object. The core region exhibits a yellowish-white hue, indicative of an older stellar population. This central bulge is surrounded by a fainter, more diffuse halo of light. There is a hint of bluer colors in the outer regions of the galaxy, potentially suggesting the presence of younger, hotter stars in these areas. The morphology suggests a smooth, elliptical-like structure, lacking prominent spiral arms or a distinct disk. There's a very slight asymmetry or minor disturbance visible, possibly from a minor gravitational interaction. The overall appearance is relatively smooth and well-defined.
