The galaxy appears to be an elongated, cigar-shaped structure, presenting itself as an edge-on spiral or lenticular galaxy. The primary body of the galaxy shows a smooth, continuous light distribution, suggesting a high degree of symmetry and a lack of significant spiral arm structures or prominent dust lanes. A gradient in the color distribution is discernible. The central region exhibits a reddish-orange hue, indicative of an older stellar population and potentially a higher concentration of dust. Progressing outwards from the core towards the extremities, the color shifts towards a bluer tone, which may be indicative of younger, hotter stars residing in a more diffuse region of the galaxy. One end of the galaxy displays a brighter and more distinct reddish region, possibly a region of increased star formation or a more concentrated central bulge of older stars. Overall, the galaxy presents as a relatively undisturbed system with no obvious signs of major mergers or tidal interactions. Minor disturbances, however, cannot be ruled out.
