The galaxy presents as a fairly smooth, elliptical structure. The central bulge exhibits a high degree of luminosity, with a gradual decrease in brightness moving towards the outer regions of the galaxy. There's little evidence of distinct spiral arms or significant dust lanes. The galaxy is not perfectly spherical, showing a slight elongation, more akin to an oblate spheroid. The color profile suggests a population of older stars, dominating the overall light output. There is no obvious sign of active galactic nuclei activity or recent major merger events.
