The galaxy presents as a single, dominant spheroid with a smooth, centrally concentrated light profile. It exhibits a yellow-white hue at the core, suggestive of an older stellar population and reduced star formation. The galaxy's apparent morphology is generally elliptical, appearing fairly round. No spiral arm structures or significant dust lanes are discernible within the image resolution. There is no apparent evidence of ongoing major merger events or tidal disturbances. The lack of strong blue color components indicates relatively low current star formation activity. A faint green and red emission is seen around the perimeter of the galaxy which suggests that star formation has stopped or is occurring in isolated pockets.
