The galaxy presents as a centrally concentrated, elliptical-like system. Its light profile appears smooth and generally featureless. The core is a bright, diffuse yellowish-white, suggesting a population of older stars. Moving outward from the core, the light becomes less intense, with a reddish-orange hue. There is no obvious spiral arm structure or evidence of active star formation. The overall morphology suggests a quiescent system with little ongoing activity. The system does not show signs of any major mergers or tidal disturbances.