The galaxy presents a generally smooth and rounded morphology. A central, concentrated bulge dominates the overall structure with a yellowish hue. The outer regions display a less intense, more diffuse greenish coloration, indicating potentially younger stellar populations in these areas. There are no readily apparent spiral arms or bar structures visible. The overall appearance suggests an evolved system, with a significant fraction of its stellar mass concentrated in the central region. The galaxy appears relatively isolated with no immediately obvious signs of ongoing major merger activity or strong tidal disturbances.
