The galaxy presents as an elongated, cigar-shaped structure. Its color profile suggests an older stellar population, with a dominant yellowish-orange hue throughout the central region. There is a hint of bluer light towards the edges, potentially indicating some ongoing, albeit minimal, star formation. The overall smoothness of the galaxy implies a lack of significant spiral arm structure or irregular features. There are no immediately obvious signs of a major ongoing merger, though subtle disturbances or tidal features cannot be ruled out given the image resolution.
