The galaxy presents as a relatively smooth, centrally concentrated object. Its morphology appears mostly elliptical, exhibiting a high degree of roundness. The central region displays a bright, yellowish hue, suggesting a significant population of older stars. There is a faint blue extension on its sides that could be a feature or disc that has been disrupted. No prominent spiral arms or significant dust lanes are readily visible. There might be some minor tidal disturbance. Overall, this galaxy appears to be a relatively quiescent system.
