The galaxy presents as a somewhat elongated, cigar-shaped structure. Its central region exhibits a bright, concentrated light, suggesting a significant stellar density or possibly an active galactic nucleus. Moving outwards from the center, the light intensity gradually diminishes, forming a more diffuse halo. There appears to be a faint, bluish tint in the outer regions, potentially indicative of younger, hotter stars and ongoing star formation. Patches of slightly redder light are also observed, hinting at the presence of older stellar populations or dust. The overall appearance suggests a galaxy with a relatively smooth structure, but there are some minor disturbances or irregularities.
