The galaxy presents as an elliptical-like structure, elongated in shape. The light distribution appears smooth, with a concentration towards the center, suggesting a central bulge or core. The color profile exhibits a gradient, with a yellowish hue dominating the central regions, shifting towards redder tones in the outer parts of the disk. No distinct spiral arms or intricate dust lanes are visible in the image. The galaxy's apparent size and shape could indicate that we're viewing a massive galaxy from a significant distance, which is experiencing an average amount of star formation. There are no apparent signs of ongoing major mergers or significant tidal disturbances.
