The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge. There is minimal visual evidence of spiral arms or a distinct disk component. The morphology appears generally rounded. The galaxy's color profile suggests a dominant population of older stars, exhibiting a yellowish hue, but the presence of some slightly bluer regions hints at the existence of some younger stars. There is no indication of any major ongoing merger events, although a slight asymmetry in the outer halo could suggest some minor gravitational interaction in its past. 
