The galaxy presents as an elliptical morphology, with a smooth, centrally concentrated light distribution. The color gradient indicates a generally older stellar population, transitioning from a yellowish core to a redder outer halo. There is no clear evidence of spiral arms or significant dust lanes. The object appears largely undisturbed, without any obvious signs of major mergers or tidal disruptions. The galaxy has a slight ellipticity, appearing somewhat flattened rather than perfectly spherical, and may be undergoing a minor interaction.
