The galaxy presents a generally smooth morphology, appearing as an elliptical or lenticular system. The central region exhibits a concentrated bright core, surrounded by a more diffuse halo. While the overall structure appears largely undisturbed, there is faint evidence of minor asymmetry or subtle irregularities in the outer regions, suggesting potential past or ongoing interactions. Color gradients appear subtle, with a central region exhibiting a yellow to reddish hue, transitioning to a slightly bluer tint in the outer regions, potentially indicating younger stellar populations in the disk. There may be subtle dust lanes or patches throughout the disc of the galaxy. This system is relatively compact.
