The galaxy appears as a relatively smooth, centrally concentrated object. Its morphology suggests an elliptical galaxy or potentially a spiral galaxy seen face-on with a dominant bulge. There is a noticeable color gradient, with a yellowish-white core transitioning to a slightly bluer outer region. This color difference could indicate variations in stellar populations, with older, redder stars dominating the core and younger, bluer stars populating the outer regions. The overall shape is mostly round. There is no obvious indication of major tidal disturbances or merging activity.
