The galaxy presents as a relatively smooth, elliptical-like structure. Its core exhibits a bright, concentrated luminosity, suggesting a significant concentration of stars within the galactic nucleus. The overall color profile is dominated by redder wavelengths, indicative of an older stellar population and/or significant dust obscuration. The galaxy shows a slight elongation and is considered relatively round overall. There appear to be no strong signs of active star formation, with any star formation that is happening occurring at low rates. There are no strong visual disturbances or tidal features to suggest a recent major merger event, however a minor disturbance is possible.
