The galaxy presents an elongated, cigar-shaped morphology. It appears relatively smooth in texture with a brighter, more condensed central region, potentially indicating a bulge. There is a hint of a disk structure, but it is not clearly defined, showing only subtle features. Color gradients are visible; the central region exhibits a somewhat bluer hue, possibly suggesting a population of younger, hotter stars. The outer regions appear redder, which could be indicative of older stellar populations or dust obscuration. There are no obvious signs of strong spiral arm structures or major disturbances, though a faint asymmetry might imply a minor interaction or past disturbance event. The galaxy appears to be relatively isolated in the image, showing no signs of an ongoing merger with another large galaxy.
