The galaxy presents as an elliptical system, exhibiting a primarily smooth morphology. The galaxy appears to be in a late stage of evolution, with low to medium star formation. The central region displays a concentration of higher luminosity, indicative of an older stellar population, while the disk shows evidence of moderate star formation. The overall shape appears to be relatively undisturbed. It has a somewhat elongated profile, more intermediate than round, with no evidence of spiral arms or a bar structure. There might be a slight distortion, suggesting a minor gravitational interaction with another galaxy. The galaxy does not show signs of major ongoing mergers or significant tidal disruption.
