The galaxy presents a generally smooth, elliptical morphology. It exhibits a distinct color gradient, transitioning from a more yellow/orange core to a bluer outer halo. The galaxy appears to be relatively isolated, with no obvious signs of major mergers or significant tidal disturbances in this image. There might be faint, subtle disturbances, but the overall impression is one of relative quiescence. The distribution of light suggests a higher concentration of older stellar populations in the central region, while younger, bluer stars seem to be more prevalent in the outer regions. The galaxy's shape is not perfectly round, showing a slight elongation, indicating a moderate degree of ellipticity.
