The galaxy appears to be a relatively smooth, elliptical type. It exhibits a centrally concentrated luminosity profile, with a bright, yellowish core that gradually fades into a diffuse halo. There is a subtle color gradient, with the core appearing more yellow, likely indicating an older stellar population, and the outer regions showing hints of bluer light, possibly suggesting the presence of younger stars or star formation regions, though such regions are not particularly prominent. The galaxy's morphology is generally rounded, lacking any distinct spiral arms or bar structures. There may be a faint tidal feature or small companion galaxy located to the upper right, warranting further investigation for signs of past or ongoing interaction. Overall, the galaxy seems to be a massive system with an estimated stellar mass of around 10^11 solar masses, and is currently undergoing a low level of star formation.
