The galaxy appears as a centrally concentrated, relatively smooth object. Its overall shape is elliptical, though not perfectly so, leaning towards being moderately round. The core exhibits a strong concentration of light, appearing distinctly brighter than the surrounding regions. The colour profile suggests a redder central population possibly indicating older stars or significant dust obscuration. There is a subtle gradient in colour as you move outwards from the core, transitioning to a slightly bluer hue in the outer regions, hinting at the possibility of younger stellar populations present at the periphery, though the level of star formation appears to be low. There is no visible evidence of a distinct disk component or prominent spiral arms. No significant mergers or major disturbances are apparent in this field. Overall the galaxy is well defined with no distortion.
