The galaxy presents a largely featureless morphology, exhibiting a smooth and rounded appearance. It demonstrates a concentrated central bulge which decreases in luminosity as it extends outwards to an indistinct edge, appearing elliptical in overall shape. Coloration suggests an older stellar population, dominated by redder hues that transition to slightly bluer shades in the outer regions. There is no discernible evidence of spiral arms or a prominent disk structure, nor are any signs of ongoing major mergers or tidal disturbances immediately apparent. There may be a minor disturbance in the overall shape of the galaxy. The galaxy demonstrates strong light, with no evident dust lanes. 
