The galaxy presents as an elliptical or lenticular type, exhibiting a relatively smooth, featureless morphology. It appears centrally concentrated with a bright nucleus and a gradual decrease in luminosity outwards to the edges. The color gradient suggests a population of older stars, particularly within the central bulge, implied by a yellow hue. The outskirts of the galaxy show a hint of bluer light, potentially indicating some residual or ongoing star formation, however at a low rate. The overall structure is fairly regular, with no obvious signs of major mergers or significant tidal disturbances; there are no tidal tails or obvious distortions in shape. The galaxy appears to be a relatively isolated system.
