The galaxy presents as a luminous, relatively smooth structure, likely elliptical in nature, though not perfectly spherical, with a slight elongation. The core is a bright, concentrated region exhibiting a yellow-orange hue, suggestive of an older stellar population. This coloration fades towards the outer regions of the galaxy, transitioning into a more diffuse, greenish-blue halo, hinting at some ongoing, though perhaps limited, star formation activity. No distinct spiral arms or bar structures are discernible. The galaxy exhibits only subtle disturbances, with no obvious signs of a major merger event in its recent past. Overall, the morphology suggests an evolved system with a substantial mass and a moderate rate of star formation.
