The galaxy presents as a centrally concentrated, elliptical-like object with a smooth, diffuse light distribution. The core exhibits a yellowish hue, suggesting a population of older stars. The overall shape appears somewhat elongated, but largely rounded. There is no obvious spiral structure or prominent dust lanes. Faint extended emissions are barely detectable beyond the central region, indicating a gradual decline in stellar density with increasing radial distance. The galaxy appears relatively undisturbed, with no apparent signs of major mergers or tidal interactions.
