The galaxy presents a largely featureless, smooth morphology. It exhibits a generally elliptical shape, appearing nearly round in projection. The light distribution suggests a centrally concentrated bulge. There is no clear evidence of spiral arms, a distinct disk, or ongoing major mergers. A very slight asymmetry might hint at minor disturbances or interactions, though this is not definitive from the available imagery. The color profile implies a population of older stars. Star formation activity is likely suppressed in this galaxy. 
