The galaxy presents as an elongated, cigar-shaped structure with a smooth overall appearance. There is an apparent lack of distinct spiral arms or a prominent central bulge. The color distribution suggests a subtle gradient, with a slightly bluer hue towards the edges and a redder tone towards the center. There is no indication of significant dust lanes or recent major merger activity. Minor asymmetry may be present in its elongated form. Overall, the galaxy appears relatively quiescent in terms of star formation.
