The galaxy appears as an elongated, cigar-shaped structure. Its central region exhibits a bright, yellowish-orange hue, suggesting a concentration of older stars. Fainter, bluish extensions are visible extending from the central bulge, hinting at possible spiral arm structures or regions of younger stellar populations. The overall morphology is relatively smooth, with no clear evidence of major disturbances or recent mergers. The galaxy has a somewhat diffuse appearance, with the outer edges gradually fading into the background sky. There is a hint of asymmetry in the outer regions, possibly indicating a minor interaction or past merger event, though further investigation is required to confirm.
