This galaxy presents as a centrally concentrated object, appearing largely smooth and elliptical in morphology. The core exhibits a bright, almost unresolved luminosity profile, indicative of a substantial stellar population density. There appears to be minimal indication of spiral arm structures or prominent dust lanes. The overall color profile suggests a relatively evolved stellar population, with a bias toward redder wavelengths. However, some blue light is observable, suggesting a small amount of ongoing star formation. There is a very slight indication of some tidal interaction or minor disturbance in the overall shape, but its overall form is predominantly spheroidal. There are no obvious signs of a major merger event in progress.
