The galaxy presents as a flattened, elongated structure, approximately cigar-shaped in appearance. A central bulge is visible, exhibiting a yellowish-orange hue, suggesting a population of older stars. The disk component of the galaxy displays a bluer color profile, indicative of younger stars and potentially ongoing star formation. There is no clear spiral arm structure, but a slight irregularity can be noticed along the edges of the disk, indicating potential disturbances or interactions with surrounding objects.
