The galaxy presents as a somewhat elliptical, though not perfectly round, structure. It exhibits a smooth, largely featureless morphology. The central bulge appears concentrated and emits light across the visible spectrum, with a yellowish-white hue. The galaxy appears relatively isolated, showing no strong signs of tidal interaction or ongoing merger events. Faint extensions of light are barely visible extending from the main body, potentially indicating a disrupted structure or interaction history. There are no distinct spiral arm features, and the light distribution falls off relatively uniformly from the center towards the edges. The color suggests a population of older stars, and indicates a low star formation rate.
