The galaxy presents as a fairly smooth, elliptical morphology. The light distribution indicates a high degree of central concentration, with a bright, well-defined core that gradually fades into the surrounding halo. There is a distinct lack of any spiral arm structures or prominent dust lanes; the overall texture appears homogenous. The color profile indicates that the galaxy is composed predominantly of older stellar populations, exhibiting a yellow to reddish hue consistent with a low rate of star formation. There's very little evidence of recent major merger events.
