This galaxy presents as an elongated, disk-like structure. The central bulge is a dominant feature, exhibiting a yellowish-orange hue, suggesting an older stellar population. The outer regions of the galaxy display a slightly bluer tint, indicating the presence of younger stars and ongoing star formation, albeit at a modest rate. The overall shape is decidedly cigar-shaped. There is no apparent interaction with any other galaxies, nor any significant disruption of its form, suggesting relative isolation and stability. There is no clear dust lane. Overall, the galaxy appears to be a relatively undisturbed system undergoing steady, low-level star formation.
