The galaxy presents as an elliptical-like structure, possibly a lenticular galaxy seen nearly face-on. Its morphology appears largely smooth, with a bright, concentrated central bulge that dominates the overall light profile. Fainter, somewhat extended and diffuse features are visible in the surrounding regions. There's an indication of some irregularity in the outer regions; this could possibly represent the presence of a faint, disturbed disk component or signs of minor interactions/merging events.

The color distribution indicates a prominent red color gradient toward the center, which suggests a population of older stars within the bulge. Hints of bluer colors are observed in the outer regions, which may indicate regions of more recent star formation. The low-contrast nature of any spiral arms could also mean that the arms are tightly wound.
