The galaxy presents as a relatively smooth, elliptical structure. It exhibits a concentrated central bulge with a yellow-orange hue, suggesting a population of older stars. There is little evidence of spiral arms or significant dust lanes. The light gradually fades from the center, indicating a fairly uniform stellar distribution across the galaxy's body. Its shape is tending more towards round, but it is not perfectly spherical. There might be a slight distortion in its outer regions, possibly hinting at a minor gravitational interaction or previous merger event, although the overall morphology appears largely undisturbed. There is some blue light visible in the outer regions of this galaxy.