The galaxy presents as a concentrated, elliptical-like structure. Its morphology appears largely smooth and lacks any prominent spiral arms or distinct features indicative of active star formation regions. The central region exhibits a bright, concentrated core that fades into a diffuse halo. The galaxy is generally round with minimal elongation. There is no evidence of ongoing or recent major merging events or significant tidal disturbances. The color profile suggests a population of older stars, with a general trend toward redder colors.
