The galaxy presents as a well-defined, elongated structure. Its central region exhibits a concentration of luminosity. The overall color gradient suggests a population of older stars dominating the core, appearing redder in hue. Extending outward from the core, the galaxy shows a transition towards bluer tones, hinting at the presence of younger stellar populations and ongoing star formation within the galactic disk. The disk appears moderately structured, without a clear spiral arm morphology visible. The galaxy has a smooth appearance, with only subtle indications of disturbances or major morphological features. Its shape is consistent with that of a cigar. The general color distribution suggests an evolving system with differing stellar populations.
