The galaxy presents as an elongated, cigar-shaped structure, with a noticeable color gradient. A concentrated yellowish core is observed, suggesting a population of older stars or dust obscuration. Fainter, bluer emissions extend from the core along the major axis of the galaxy. These blue regions likely indicate areas of active star formation within the galaxy. The overall structure appears relatively smooth, however a slight disturbance can be observed with the presence of a long, bright extension, possibly a tidal tail, suggesting a past interaction or merger event with another galaxy.
