The galaxy appears as a centrally concentrated object with a smooth morphology. The central region exhibits a bright, yellowish-white hue, suggesting a population of older stars. Moving outward from the core, the light gradually fades, with a slight elongation along a particular axis, indicating it is not perfectly circular. The galaxy seems to be relatively isolated, with no obvious signs of major tidal disturbances or ongoing mergers. There might be a very faint disk, but it is not clearly seen due to the limitations of the image quality. Overall, it resembles an elliptical galaxy at an approximate distance that places it at a moderate redshift.
