This galaxy presents as a relatively smooth, elliptical system with a high degree of central concentration. The light distribution appears fairly uniform, with a bright, compact core that decreases in intensity outwards. The overall shape is somewhat elongated, exhibiting a moderate axis ratio but without any discernible spiral arm structures or prominent dust lanes. Color gradients suggest a population of older stars, contributing to the overall reddish-yellow hue, though a small amount of bluer light is visible in the outer regions, possibly indicating pockets of younger stellar populations. There are no obvious signs of ongoing major mergers or tidal disturbances, although a subtle asymmetry in the outer halo may indicate minor interaction history.
