The galaxy presents as a relatively smooth, centrally concentrated object with a roughly elliptical morphology. There is a subtle color gradient visible, transitioning from a slightly bluer hue at the periphery to a more yellow-red color towards the core. No distinct spiral arms or prominent dust lanes are apparent. There is a slight deviation from perfect roundness, with the shape appearing subtly elongated. No signs of major mergers or significant tidal disturbances are visible in the immediate vicinity of the galaxy. Based on the color indices, it appears the galaxy is likely a luminous and relatively massive system, although its current star formation rate is not particularly high.
