The galaxy appears as a somewhat face-on spiral or lenticular system, exhibiting a moderately bright, centrally concentrated bulge. The bulge exhibits a color gradient, transitioning from a yellowish-white core to a bluish hue in the surrounding regions. There is evidence of a disk structure surrounding the bulge, exhibiting hints of spiral arm formations, although the arms are not sharply defined, suggesting they are likely tightly wound. Color variations across the disk indicate regions of active star formation, especially in the bluer areas. The overall structure does not suggest a recent major merger event, but the possibility of minor interactions or past disturbances cannot be ruled out.
