The galaxy presents as an elongated, cigar-shaped structure. It exhibits a relatively smooth, diffuse light distribution with a concentration towards the center. The color gradient appears to be subtly bluer at the core, transitioning to slightly redder hues in the outer regions. There is no strong evidence of spiral arms or distinct features such as dust lanes or prominent star-forming regions discernible in this image. Minor distortions and irregularities are present, possibly suggesting some recent interaction or minor disturbance. There is no single, dominant nucleus, but rather a blended central bulge region. The galaxy appears relatively isolated, with no immediately apparent interacting companion galaxies.
