The galaxy presents as a relatively smooth, elliptical morphology. The central region exhibits a high concentration of light, indicating a prominent galactic nucleus or bulge. The galaxy appears generally round, lacking any strong evidence of spiral arm structure or significant tidal disturbances. The color profile suggests a population of older stars, with a dominant yellowish-orange hue, indicative of lower ongoing star formation. There are some bluer, brighter spots within the galaxy which are indicative of some star formation. Overall, this galaxy appears to be an evolved system.