The galaxy presents as a smooth, elliptical-like structure. It exhibits a concentrated central bulge that transitions to a diffuse outer halo. The core is characterized by a yellowish-white hue, potentially indicating an older stellar population. The outer regions show hints of bluer light, suggesting the presence of some younger stars or ongoing star formation. The overall shape is elongated, displaying a cigar-like morphology. There is no obvious indication of spiral arms, a bar structure, or any significant tidal disturbances, suggesting the absence of recent major merger events. The smoothness of the light distribution and color gradients suggests an evolved system, likely with a considerable stellar mass.
