This galaxy exhibits a generally smooth morphology, with a hint of a disk-like structure. The galaxy's shape is elongated, appearing more cigar-shaped than perfectly round. The central region presents a brighter, concentrated luminosity, indicative of a galactic bulge. The outer regions of the galaxy appear more diffuse and less structured. No major mergers or significant disturbances are immediately apparent in this image. There is evidence of ongoing star formation, with regions appearing to have a slightly blueish-green tint, which may indicate younger, hotter stars.
