The galaxy presents as a relatively smooth, centrally concentrated structure with a slight ellipticity. The core exhibits a reddish hue, potentially indicating an older stellar population or dust obscuration. Moving outwards, the color profile shifts to a bluer tone, possibly indicative of younger stars. There appears to be a slight disturbance in its morphology, but no prominent features, such as spiral arms or a distinct disk. The light distribution is quite diffuse, suggesting a relatively high level of homogenization. Its overall appearance leans toward that of an elliptical galaxy, although some minor features suggest it is not a perfect sphere. The galaxy appears largely isolated with no signs of a major ongoing merger. 
