The galaxy appears to be a relatively smooth, centrally concentrated system. Its morphology suggests an elliptical classification, showing a predominantly spheroidal shape with a lack of apparent spiral arms or a well-defined disk. There is a bright core indicating a high concentration of stars or possibly an active galactic nucleus, gently fading to a dimmer halo. The overall color appears to be on the redder side, hinting at a potentially older stellar population with reduced current star formation. There is no readily apparent tidal debris, significant dust lanes, or signs of ongoing major merger activity, with only minor indications of asymmetry or disturbances in the outer regions. It is a fairly compact system, with light concentrated towards the central region.
