The galaxy presents as an elliptical morphology, with a smooth, diffuse light distribution indicative of an older stellar population. A centrally concentrated bulge is clearly visible, exhibiting a yellowish-white hue, suggesting a dominance of evolved stars. The overall color gradient suggests a general decrease in blue light toward the galactic center. The outer regions appear fainter and less defined, with a hint of a disk-like structure. There is a possibility of minor disturbances or faint tidal features hinting at past or ongoing interactions, but they are not definitively visible. The galaxy does not show a well-defined spiral structure.
