The galaxy appears to be an elliptical galaxy, presenting a relatively smooth and concentrated light profile. It exhibits a bright, moderately compact core, potentially indicative of a supermassive black hole or a dense stellar population at its center. Moving outward from the core, the light gradually diminishes, forming a diffuse halo. The overall shape tends towards elliptical, but with some deviation, appearing more 'in-between' elliptical and spherical than clearly one or the other. There is some evidence of asymmetry, a possible slight disturbance or minor interaction. The galaxy displays a range of colors, from a reddish-yellow core to a bluish halo, suggesting varying stellar populations, with older, redder stars concentrated in the center and younger, bluer stars in the outer regions, which is consistent with an undergoing, yet mild, star-formation activity.
