The galaxy presents as a somewhat diffuse object, exhibiting a roughly elliptical morphology. A central, brighter region suggests a galactic nucleus. The overall color profile indicates a mix of stellar populations, with a central region exhibiting warmer, yellower tones, potentially indicative of older stars. There are hints of bluer regions in the outskirts. The overall structure suggests a relatively massive system. The galaxy appears relatively isolated with no clear signs of major disturbances or ongoing merger activity.
