The galaxy presents as a centrally concentrated object with a generally smooth morphology. The core region exhibits a yellowish hue, possibly indicating an older stellar population. Surrounding the core, a fainter, diffuse halo is visible, displaying subtle color variations, transitioning towards bluer tones at the periphery. There is no apparent spiral structure or distinct disk features discernible in this image. The overall shape approximates a rounded form with a hint of elongation. There is no obvious sign of tidal disruption or ongoing major merger events. However, very slight asymmetries in the outer halo cannot be ruled out. The galaxy is relatively compact, with the majority of its light concentrated within a small radius.
