The galaxy presents as an elongated, cigar-shaped structure. It appears relatively smooth, with a bright, concentrated central bulge that gradually diffuses outwards. There is a subtle color gradient observed from the center to the outer edges. The core region presents a reddish hue, possibly indicative of an older stellar population. Fainter bluish tinges are observed within the galaxy's disk, hinting at regions of possible star formation. There is no obvious presence of spiral arm structures or prominent dust lanes. Overall, the galaxy's morphology is consistent with that of an early-type spiral galaxy or an elliptical galaxy viewed edge-on.
