The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a concentrated central bulge, appearing nearly spherical. A slight elongation is possibly present, but it is close to round. There are no clear indications of spiral arms or a distinct disk component within the observed image. The galaxy appears to be relatively isolated, showing no major signs of ongoing mergers or significant tidal disturbances. The color gradient suggests an older stellar population dominating the galaxy's composition, particularly within its central regions. There is some evidence of a fainter halo surrounding the main body, though its extent is not well-defined.
