The galaxy exhibits a lenticular morphology, appearing as a flattened disk with a bright, prominent bulge at its center. The bulge appears yellowish-white, suggesting an older stellar population. A disk extends outwards from the bulge, showing a subtle color gradient from yellowish near the center to slightly bluer at the edges. The disk appears relatively smooth, with minimal evidence of spiral arms or significant dust lanes. The overall shape of the galaxy is elongated, appearing cigar-shaped, suggesting an inclined viewing angle relative to the galactic plane. There is no obvious presence of a major ongoing merger or tidal disturbance.
