The galaxy presents a generally elliptical morphology. Its core exhibits a bright, concentrated luminosity profile, transitioning smoothly into a more diffuse halo. The galaxy appears somewhat elongated along a principle axis. Within the halo, hints of finer structure are observed; subtle color variations suggest differential stellar populations. The object lacks prominent spiral arm structures or features indicative of active star formation regions, such as HII regions. The overall color indices suggest a relatively old stellar population, which is consistent with its smooth morphology. There is very little evidence of ongoing merger activity or galactic disruption.
