The galaxy presents as a relatively smooth, elliptical structure. Its light distribution appears centrally concentrated, with a gradual decrease in luminosity towards the outer regions. There is little evidence of spiral arms or significant dust lanes. The core region seems to emit a yellowish light, while the outer regions appear a little redder, suggesting a population of older stars. There is little to no indication of any major recent merger events or strong tidal interactions. The morphology indicates a high likelihood of being classified as an elliptical galaxy with no distinct features. The galaxy displays no strong blue light indicative of recent star formation.
