The galaxy appears as a fairly smooth, elliptical structure. The central bulge exhibits a yellowish hue, suggesting an older stellar population, while the outer regions are slightly bluer, potentially indicating more recent star formation. There is no obvious spiral arm structure, and the overall morphology leans towards an elliptical shape. The galaxy's form suggests a relaxed system, possibly having undergone multiple merger events in its past, leading to its current smoothed appearance. Minimal dust lanes are apparent, and the light distribution indicates that the galaxy's shape is somewhere between round and elongated. There is no clear indication of tidal disturbances or ongoing major mergers from its immediate appearance.
