The galaxy presents as a relatively smooth and centralized distribution of light. The core exhibits a bright, concentrated luminosity, suggestive of a significant stellar population density. Proceeding outward from the nucleus, the light gradually diffuses, forming a flattened, elliptical shape. The major axis appears to be several times longer than its minor axis, hinting at a moderate degree of ellipticity. The overall color appears yellow-orange, perhaps indicating an older stellar population with a lower rate of ongoing star formation, though there may be pockets of bluer light in the outer regions, possibly suggesting some presence of younger stars. There is no apparent spiral structure, or strong signs of tidal disturbances, implying it may have undergone recent mergers.
