The galaxy presents a generally smooth, elliptical morphology. The core exhibits a concentrated luminosity profile, appearing as a bright, nearly unresolved center. Moving outward from the core, the light gradually diminishes, with no distinct spiral arms or bar structure visible. There is a subtle color gradient, with a yellowish-white core transitioning to a bluer hue in the outer regions. This color difference potentially indicates variations in stellar populations, with older stars concentrated toward the core and younger, hotter stars more prevalent in the outskirts. There is little evidence of active merging or major disturbances.
