The galaxy appears to be a spiral type, viewed at a significant angle relative to its plane. It exhibits a central bulge that appears somewhat indistinct and asymmetrical. The spiral arms are not clearly defined, suggesting either a flocculent structure or a more distant, faint galaxy. There is evidence of possible minor disturbances or interactions, evidenced by the slight asymmetry in the arm structure on one side of the galaxy, and a faint plume-like extension emanating from one end. The disk component is visible, though patchy. Star formation regions appear to be sparse and not particularly bright or numerous. Overall, the galaxy presents an intermediate morphology, not clearly elliptical nor a grand design spiral, and exhibits hints of potential interactions.
