The galaxy presents as a relatively smooth object with an elongated, cigar-like morphology. There is a noticeable color gradient across the galaxy, transitioning from a bluer hue at the outer edges to a more yellow/red tinted central region, indicating either a difference in stellar populations or dust absorption. There is little to no visible structure such as spiral arms or distinct star-forming regions. The galaxy appears to be relatively isolated, showing no clear signs of major interactions or merging events. The smooth appearance and color profile suggest a relatively evolved system with a substantial population of older stars. The galaxy's orientation appears to be nearly edge-on.
