The galaxy appears as a single, luminous entity with a concentrated central bulge. There is a smooth transition in luminosity from the core outward, suggesting a lack of distinct spiral arms or features. The galaxy exhibits a generally elliptical shape, with a high degree of circularity. The color profile indicates a dominance of older stellar populations, with a yellow-red hue intensifying toward the core. Slight blue tinges on the periphery could suggest some ongoing, though likely minimal, star formation in these outer regions. Overall, the galaxy presents a morphology consistent with an elliptical galaxy or a lenticular galaxy seen at a significant distance, with no obvious signs of recent major mergers or tidal disturbances.
