The galaxy presents as a spiral, viewed at an oblique angle, though not quite edge-on. A prominent disk structure is visible, with a central bulge that is noticeable but not overwhelmingly dominant. The spiral arms are well-defined and exhibit a clumpy appearance, suggesting active star formation regions within them. These regions appear bluer in color, indicative of younger, hotter stars. The overall color of the galaxy suggests a mix of stellar populations, with the bulge region appearing somewhat redder, potentially indicating older stars or dust obscuration. The galaxy is relatively isolated, with no obvious signs of major mergers or interactions, though a minor disturbance or tidal feature cannot be ruled out based on this image alone. The galaxy exhibits no strong central bar structure. The overall morphology suggests a spiral galaxy with a moderate bulge and significant ongoing star formation.
