The galaxy presents as a centrally concentrated object, with a smooth, diffuse morphology. The core exhibits a bright, near-white luminosity, suggesting a high density of stars. Moving outward from the core, the luminosity gradually diminishes, transitioning into a more extended halo. The overall shape of the galaxy appears to be approximately elliptical, presenting a somewhat rounded appearance, without any significant features that would clearly indicate a spiral structure or a highly elongated shape. There is a slight color gradient, with the central region exhibiting a yellowish hue, transitioning toward redder tones in the outer regions. The smooth texture of the light distribution suggests it is likely an elliptical galaxy, or potentially a lenticular galaxy viewed nearly face-on. There is no prominent evidence of ongoing or recent major mergers or tidal disturbances, though some subtle irregularities might be present, hinting at a possibility of minor disturbances in its past. The image lacks clear signs of distinct spiral arms or prominent dust lanes.
