The galaxy presents a somewhat diffuse morphology. It appears largely smooth in overall structure, with a concentrated central region. The shape is approximately elliptical, trending towards a more disk-like structure when considering the galaxy as a whole. A slight blue hue dominates the outer regions, suggesting the presence of younger stars or active star formation regions. There is a faint hint of reddening or dust obscuration closer to the galactic center, evidenced by the subtle change in color gradient. No prominent spiral arms or bar structures are discernible. The overall appearance suggests a galaxy that has experienced some past interactions or minor disturbances, but is generally relatively quiescent. The absence of strong tidal features indicates no ongoing major merger events.
