This galaxy exhibits a clear disk morphology, appearing close to edge-on. There is a notable central bulge, which appears a yellowish-orange hue, indicating a population of older stars. Emanating from the central bulge, the disk presents a complex structure. One side displays a dust lane with an orange glow, suggesting active star formation. On the opposite side, a blue tinge is present, indicative of recent or ongoing star formation, where hot, young stars are present. There is an arm like feature extending far from the disk, this may indicate a tidal tail, potentially the result of a gravitational interaction or merger. The presence of both dust lanes and stellar populations of varying ages points to a dynamic system with on going evolution.
