The galaxy presents a somewhat elongated, cigar-shaped morphology. A prominent central bulge exhibits a yellowish-orange hue, suggesting an older stellar population. Fainter, bluish extensions emanate from either side of the central region, potentially indicating regions of more recent star formation within a disk-like structure. There appears to be a slight asymmetry in the distribution of light, with a possible minor disturbance observable on one side. Overall, the galaxy appears to be undergoing some level of activity, but displays characteristics consistent with both smooth, evolved stellar populations and regions of active star formation.
