This galaxy presents a generally smooth morphology, exhibiting a flattened, cigar-shaped form. The central region displays a concentrated luminosity, appearing as a bright, yellowish core. Progressing outwards from the core, the intensity of light diminishes into a diffuse, bluish halo. Though smooth overall, there's some slight evidence of internal structure within the fainter halo. No apparent signs of major mergers or significant tidal disturbances are visible, although minor disturbances cannot be entirely ruled out at this resolution. The color gradient suggests potential differences in stellar populations, with a more evolved, older population likely dominating the central core, and younger, bluer stars possibly contributing to the extended halo.
