The galaxy appears to be elliptical in shape, with a smooth and relatively featureless morphology. Its color profile indicates a dominant population of older stars, contributing to the yellowish-red hue observed in the image. There is no discernible evidence of spiral arms or a prominent dust lane. The galaxy exhibits a high degree of radial symmetry, with the light intensity gradually decreasing from the center outwards. No signs of any major ongoing mergers or tidal disturbances are visible.
