The galaxy presents a smooth, elliptical morphology, appearing largely featureless. Its color profile suggests a population of older stars, with a subtle concentration of yellow-red hues toward the galactic center. The galaxy has a very slight deviation from being perfectly circular, appearing to be an in-between shape. There is no readily apparent spiral structure or distinct dust lane visible in this observation, and no indication of any ongoing major merging activity. There are also no signs of merging or tidal disturbances.
