The galaxy presents a predominantly smooth morphology, appearing largely featureless. Its overall shape is elliptical, exhibiting an intermediate degree of ellipticity, falling somewhere between round and elongated. The central region displays a concentrated luminosity, transitioning to a fainter halo. Coloration suggests a primarily older stellar population, with a yellowish-orange hue dominating, indicative of evolved stars. There is little to no evidence of spiral arms or dust lanes. No signs of major mergers or tidal disturbances are readily apparent; any interaction is likely subtle or has occurred in the distant past. The galaxy appears relatively isolated.
