The galaxy presents as a reddish-yellow elliptical object with a moderate axial ratio, appearing somewhat flattened. Its light profile suggests a centrally concentrated luminosity distribution that decreases steadily outward. There is faint indication of a diffuse halo extending beyond the main body of the galaxy, but it lacks any distinct substructure such as spiral arms or prominent dust lanes. The overall morphology is quite smooth, with minimal evidence of recent merger activity or significant star formation. The observed color suggests an older stellar population, relatively depleted of young, massive stars.
