The galaxy presents as a centrally concentrated, relatively smooth object with a subtle, disk-like morphology. It appears nearly circular, with a slight elongation that may indicate it is more oblate in three dimensions. The galaxy exhibits a colour gradient, appearing slightly bluer in the central regions. The outer regions are fainter and redder, suggesting an older stellar population. There are no obvious signs of major mergers or significant tidal disturbances. The galaxy is relatively isolated, with no other nearby galaxies appearing to significantly impact its morphology. There is a faint, unresolved halo surrounding the core of the galaxy.
