The galaxy presents a smooth, largely featureless morphology. It exhibits a centrally concentrated luminosity profile, characteristic of an elliptical galaxy or a lenticular galaxy seen face-on. The core region displays a yellowish hue, potentially indicative of an older stellar population with lower rates of on-going star formation. The galaxy's shape appears approximately round. There are no readily apparent signs of tidal disturbances or merging activity. It is a relatively massive galaxy, with the bulk of its stellar mass concentrated in a spheroidal structure. Any spiral arms are tightly wound or absent altogether.
