The galaxy presents a generally elliptical morphology, although a slight disk-like structure is discernible. The central bulge appears bright and concentrated, with a yellowish hue, suggesting an older stellar population. Surrounding the core, a fainter and more diffuse disk is visible, exhibiting a greenish tint which hints at more recent star formation activity. The overall structure appears relatively undisturbed, with no strong signs of tidal features or major mergers. There is a slight asymmetry in the distribution of the greenish emission across the disk, potentially indicating an ongoing minor interaction or internal dynamical process.
