The galaxy presents as an elongated, cigar-shaped structure. It appears to be relatively massive, with a significant stellar population. A central bulge is visible, exhibiting a yellowish-orange hue, suggesting an older stellar population. The disk component is also apparent, showing a bluer color compared to the bulge, indicating the presence of younger stars and ongoing star formation. The galaxy exhibits some signs of disturbance, with a potential minor asymmetry, perhaps due to a past interaction or merger event. Star formation activity is present, although it is not extremely vigorous.
