This galaxy presents as an elliptical or lenticular morphology, exhibiting a smooth, relatively featureless light distribution. The light profile suggests a concentration of luminosity towards the core, diminishing gradually outward. The overall shape is elongated, with the longest axis being several times larger than the shortest axis. The galaxy displays a moderate color gradient. The central region appears yellowish-white suggesting an older stellar population and minimal ongoing star formation. The outer regions appear slightly bluer, hinting at a younger stellar population, although the overall color indicates that star formation is not dominant. No distinct spiral arms or prominent dust lanes are discernible. There is no evidence of any major merger events or significant tidal disturbances. Based on the observed shape and color properties, this galaxy is classified as a relatively evolved system that is in a relatively undisturbed state.
