The galaxy appears as a centrally concentrated object with an overall smooth morphology. The light profile suggests a relatively undisturbed system with no prominent spiral arms or significant irregular features visible in this image. It exhibits a somewhat elliptical shape, leaning toward a rounder appearance rather than a highly elongated form. The core region is distinctly brighter, likely indicating a concentration of older stellar populations, while the outer regions show a gradual decrease in luminosity. There may be a hint of subtle color variations, possibly indicating areas with differing star formation activity. No obvious signs of major mergers or tidal disturbances are readily apparent.
