This galaxy appears to be an elliptical type, exhibiting a generally smooth and centrally concentrated light distribution. Its overall shape is somewhere between round and elongated, showing a slight preference for an in-between elliptical form. The core is a bright, concentrated yellowish-white, suggesting an older stellar population dominating the nuclear region. Fainter and more diffuse light extends outwards from the core, with hints of a slight disk-like morphology. There are no obvious signs of spiral arms or significant dust lanes visible. A subtle blue shift in hue is visible moving away from the core, suggesting a slight variation in the stellar populations. There are no apparent major disturbances or ongoing major merger events affecting the galaxy's overall structure, but minor tidal interaction can not be ruled out.
