The galaxy presents as a single, largely homogenous object. Its morphology is dominated by a smooth, elliptical profile, exhibiting a high degree of circularity. The light is concentrated towards the core region, with a gradual decrease in intensity outward, lacking prominent spiral arms or distinct features within the visible spectrum. The central region appears yellowish-white, suggesting a population of older stars, while the outer regions exhibit a slightly bluer hue, perhaps indicating some ongoing, though modest, star formation. There is no clear evidence of major tidal disturbances or ongoing mergers.
