The galaxy presents as a centrally concentrated, elliptical-like system. It exhibits a smooth, largely featureless morphology, lacking any prominent spiral arms or distinct disk structures. The light distribution appears predominantly spheroidal, with a high degree of central concentration. There's a noticeable color gradient, with the core appearing more yellowish-orange, suggesting an older stellar population, while the outer regions display slightly bluer hues, indicative of the presence of younger stars. The overall shape is quite regular and rounded, with no signs of significant tidal disturbances, ongoing mergers, or major morphological asymmetries. Faint, diffuse extensions may be present, but these are minimal and blend gradually into the background sky.
