The galaxy appears to be a relatively smooth, elliptical-like structure. It exhibits a concentrated central bulge, which gradually diffuses outwards. The color profile appears consistent, trending towards a reddish-yellow hue. There are no visible spiral arms or prominent dust lanes. The galaxy appears largely undisturbed, showing no obvious signs of ongoing major merger activity or tidal distortions. It has a high degree of circular symmetry. The light distribution suggests that the stellar population is largely composed of older stars.
