The galaxy appears to be an elliptical galaxy, exhibiting a largely smooth morphology. There is little evidence of spiral arms or significant dust lanes. The central bulge is prominent and relatively bright, transitioning gradually to a more diffuse outer halo. The color gradient suggests an aging stellar population, with a yellowish hue dominating the central region, possibly indicating a higher concentration of older, cooler stars. There is a slight reddening of the central light, indicative of a higher concentration of older stars. The overall shape is close to circular, with a suggestion of slight ellipticity but lacking any obvious signs of tidal disturbances or interactions with other galaxies. Based on its apparent size and structure, it is a galaxy of significant mass, with a low rate of current star formation.
