The galaxy presents as a relatively smooth, centrally concentrated object with a near-circular morphology. The light profile appears to decline steadily from the bright nucleus outwards, lacking any distinct spiral arm features or a prominent disk component. There are no obvious signs of recent major mergers or tidal disturbances in the immediate vicinity. The galaxy exhibits a slight elongation, but it is nearly face-on. The color profile shows a moderate gradient, with the central regions appearing bluer than the outer parts of the galaxy, possibly indicating younger stellar populations in the core. The extended halo is relatively faint and smooth.
