The galaxy appears to be a relatively smooth, elliptical galaxy, with a notable bulge dominating the central region. The light is concentrated towards the core, exhibiting a centrally bright and diffuse structure. The isophotes appear largely regular, with a fairly round morphology, though some minor deviation from perfect circularity is observed. The galaxy displays a gradual decrease in surface brightness from the center outwards, with no distinct spiral arm features or prominent dust lanes visible. The overall color appears yellow-white, consistent with an older stellar population. There is no obvious indication of ongoing major merger events. Evidence suggests that it is a fairly massive galaxy.
