The galaxy appears as a relatively smooth, elliptical-like structure with an elongated shape. Its core is a bright, concentrated yellowish-white hue, indicative of an older stellar population, likely dominated by red giant stars. Extending outward from the core, a fainter, diffuse halo exhibits a slight blueish tint. This suggests the presence of a younger, hotter population of stars in the outer regions, even though the galaxy is mostly composed of older stars. There is no evidence of strong spiral arms or a well-defined disk. The overall structure suggests it is undergoing some minor gravitational disturbance, but is mostly stable.
