The galaxy presents an elliptical morphology, characterized by a centrally concentrated luminosity profile that diminishes gradually towards the periphery. The core exhibits a yellowish hue, indicative of an older stellar population. Fainter, diffuse bluer regions can be observed. It has a smooth texture and a somewhat elongated shape. There is no clear evidence of spiral arms or significant dust lanes. Indications of mild gravitational disturbances are potentially present. Overall, the galaxy appears to be a relatively evolved system.
