The galaxy presents an elliptical morphology, appearing mostly smooth. The central bulge exhibits a bright, concentrated luminosity, transitioning into a more diffuse halo. A subtle disk structure is suspected, oriented horizontally, suggested by faint extensions of bluer light emanating from the central region. The color distribution displays a gradient, with the core exhibiting a yellow hue. The outer regions show traces of redder light, possibly indicative of older stellar populations. Evidence for spiral arm structure or significant dust lanes is not apparent. The overall shape suggests a possible early-type galaxy. There is no obvious sign of major disturbance or interaction.
