The galaxy presents as an elliptical morphology. It exhibits a high degree of central concentration with a smooth light distribution. The isophotes are generally rounded, trending toward elliptical rather than disk-like or irregular. There are no apparent spiral arm structures or prominent dust lanes. The color profile suggests a population of older stars, with a yellowish-red hue dominating the core region, which extends outward to a halo of blue stars. There is a small chance of a minor galactic interaction that is causing the slightly disturbed shape in the halo.
