The galaxy presents as a somewhat elongated, elliptical or lenticular structure, exhibiting a smooth, centrally concentrated light profile. The core appears yellowish-orange, indicative of an older stellar population dominated by red giants and lower-mass stars. There is little evidence of spiral arms or significant dust lanes. The galaxy has an apparent axis ratio suggesting it is viewed at an angle. No clear signs of active star formation are visible across the galaxy's extent. The overall morphology suggests a galaxy that is relatively quiescent in terms of star formation and potentially has undergone significant evolutionary processing, resulting in a smoother distribution of stellar light and gas.
