The galaxy presents as a centrally concentrated, elliptical morphology with a smooth appearance. The core is a bright yellow, indicating a population of older stars. The outer regions fade into a reddish hue, suggesting a decreasing density of stars towards the galaxy's edge, and potential redshifting of light due to distance. There is no distinct disk structure visible. There is no visible active star formation. The overall shape appears to be somewhat rounded, with no signs of significant tidal disturbances or ongoing mergers. The galaxy appears relatively isolated and well-defined.
