The galaxy presents as a relatively smooth, elliptical-like object. Its morphology suggests a predominantly bulge-dominated system with little to no discernible spiral arm structure. The color profile indicates a population of older stars, seen in its redder hue, potentially implying lower rates of current star formation. The roundness of the galaxy suggests it is likely an E0-E3 type elliptical galaxy. There are no visible signs of major interactions or mergers with other galaxies. The galaxy is unresolved in this image.
