The galaxy presents as a largely smooth, elliptical-like structure with a concentrated central bulge. The light distribution suggests minimal evidence of spiral arms or significant disk features. There appears to be a very slight elongation, but the galaxy is mostly rounded in appearance. The central region displays a bright, concentrated intensity, indicative of a high density of stars. There are suggestions of minor irregularities in the outer regions, possibly due to interactions, but the galaxy generally exhibits a quiescent, non-disturbed morphology. The color profile indicates a relatively red population, which may suggest a lack of ongoing active star formation.
