The galaxy presents an elongated, cigar-shaped morphology. Its light profile appears relatively smooth, without obvious spiral arms or significant dust lanes. The central region exhibits a brighter, more concentrated luminosity, potentially indicative of a galactic bulge or a more densely packed stellar population. There is a color gradient evident from the center outwards, with a slightly more reddish hue concentrated towards the bulge, transitioning to a bluer, whiter color in the outer regions. This could suggest ongoing star formation in the galaxy's disk, or a population of younger, hotter stars. The galaxy does not show clear signs of major disturbances or mergers based on its regular shape.
