The galaxy appears to be an elliptical galaxy, displaying a generally smooth and concentrated light profile. The central region is significantly brighter, exhibiting a yellowish-orange hue. Moving outwards from the core, the light intensity diminishes gradually. No distinct spiral arms or other detailed features are discernible. There appears to be a slight elongation, but the galaxy is largely spheroidal. The color suggests an older stellar population. Star formation appears to be occurring at a low rate within this galaxy. No signs of a recent or ongoing merger can be observed; the morphology is relatively undisturbed.
