The galaxy presents as a centrally concentrated object, appearing largely smooth in morphology. The light distribution suggests a spheroidal shape, with a high degree of roundness and minimal elongation. There is no clear evidence of spiral arms, a distinct disk, or any significant features indicative of recent or ongoing mergers or tidal disturbances. The galaxy exhibits a color gradient, with a yellowish hue dominating the central region, transitioning to slightly bluer tones towards the outer edges. This color variation might reflect differences in stellar populations, with older, redder stars concentrated towards the center and younger, bluer stars possibly residing in the outskirts. The overall appearance suggests that star formation is occurring at a low rate, consistent with an evolved or quiescent galaxy.
