The galaxy presents as a relatively smooth, elliptical-like structure with a high degree of central concentration. The light distribution is centrally peaked, exhibiting a gradual decrease in surface brightness from the core outwards. There is little evidence of spiral arms or prominent dust lanes. The galaxy appears mostly homogeneous in color, displaying a primarily yellowish-white hue suggesting an older stellar population, with minimal indication of ongoing, active star formation. It appears fairly symmetrical and the disk has a slight degree of ellipticity to it. There appears to be little or no evidence of any tidal disturbances, suggesting it has not undergone a major merger recently.
