The galaxy presents as a generally smooth, elliptical form. There is a distinct central bulge exhibiting a yellow-orange hue, suggesting a population of older stars. A faint, diffuse halo surrounds the central region, with a subtle greenish tinge, which may indicate the presence of a younger stellar population or ongoing, albeit weak, star formation. There is no indication of spiral arm structure, bars, or significant dust lanes. The overall morphology suggests a relatively evolved system with minimal recent merger activity.
