The galaxy presents an elliptical morphology, appearing largely smooth and featureless in the image. The light is concentrated towards the center, forming a bright, relatively compact core. The overall color profile suggests a population of older stars dominating the stellar content, giving it a slightly redder hue at the edges while the core has an intense blue hue. There is no apparent spiral arm structure or significant dust lane visible. The galaxy exhibits a high degree of symmetry, with a generally rounded, though slightly elongated, shape. There are no obvious signs of ongoing major mergers or tidal disturbances.
