The galaxy appears as a relatively smooth, elliptical-like structure with a concentrated central bulge. It exhibits a gradual decrease in luminosity from the core outwards. The color profile suggests a population of older stars with a redder hue dominating the overall light. There is little evidence of distinct spiral arms or dust lanes. The galaxy's shape is nearly circular, exhibiting a high degree of central symmetry. There are no obvious signs of major ongoing merger activity, though subtle disturbances cannot be ruled out.
