The galaxy presents as a smooth, elliptical structure. It exhibits a concentrated central bulge, with a gradual decrease in luminosity moving outward. The color profile suggests a population of older stars, indicated by a yellow-red hue in the central region. The galaxy's shape is elongated, with a major axis significantly larger than its minor axis. There is a faint disk like structure, but it is difficult to make out in detail. There is no evidence of spiral arms or active star formation regions. The galaxy appears relatively undisturbed.
