The galaxy appears to be an elliptical galaxy, exhibiting a smooth, centrally concentrated light profile. It presents a relatively round shape, although there is a slight suggestion of elongation along one axis. No distinct spiral arms or other prominent features are discernible. Color gradients are subtle, showing a slightly more yellow hue towards the central regions, possibly indicating an older stellar population. There is no evidence of ongoing major mergers, though subtle disturbances could be present. Based on its color and morphology, this galaxy is likely a relatively massive system with a suppressed star formation rate.
