The galaxy presents a largely smooth morphology, with a centrally concentrated luminosity profile, likely indicating a dominant bulge component. The core exhibits a yellowish hue, transitioning to a bluish-green towards the outer regions. This color gradient suggests a possible variation in stellar populations, with older, redder stars concentrated in the bulge and relatively younger, bluer stars occupying the disk. The overall shape appears to be elliptical, exhibiting very little disk-like feature or signs of spiral arms. The morphology is most consistent with an early-type galaxy, possibly an elliptical or lenticular galaxy. There are some very minor disturbances observed.