The galaxy presents an elongated, cigar-like morphology. The central region exhibits a yellowish-orange hue, possibly indicating an older stellar population. This core appears relatively smooth and concentrated. Moving outwards from the center, there is a fainter, more diffuse region. There are no distinct spiral arms or a well-defined disk. The galaxy seems to be undergoing a possible merging event, with a portion of the galaxy appearing somewhat disturbed and asymmetric. Overall, the galaxy lacks strong blue color, suggesting lower current star formation activity.
