The galaxy appears to be an elliptical galaxy, exhibiting a smooth, relatively featureless morphology. The light distribution suggests a high degree of central concentration, with a bright core that gradually diminishes outwards. The overall shape appears to be generally round. There might be some faint distortions in the outer regions, possibly indicating past minor gravitational interactions or mergers. The color profile appears to be redder in the central regions, transitioning to slightly bluer hues in the outskirts, suggesting an older stellar population towards the core and a potentially younger population in the outer regions. Overall, the galaxy appears to be in a relatively settled state, with limited evidence of significant ongoing star formation.
