The galaxy exhibits a primarily smooth morphology with what seems to be a disk feature. The central region presents a bright, concentrated luminosity. There is evidence of a possible faint ring structure surrounding the central bulge. A subtle asymmetry is present in the outer regions of the disk, possibly indicating a past or ongoing minor interaction, or internal disturbances. The colour profile transitions from a bluer hue in the central region to a redder hue at the edges of the disk.
