The galaxy presents as a relatively small, elongated object with a cigar-like shape. The central region appears smoother and more concentrated, possibly indicating a bulge or nucleus. The disk is oriented edge-on relative to our line of sight, with a slight tilt visible. There is a hint of structural irregularity or minor disturbance, possibly indicative of a past interaction or merger. The overall color suggests a population of older stars, with a relatively low rate of star formation, but there are pockets of blue light suggesting some ongoing star formation, although minimal. The galaxy appears to be generally isolated, without any prominent companion galaxies nearby.
