The galaxy presents as a concentrated central region of high luminosity, suggesting a significant stellar population. The core appears predominantly yellow/white in color, potentially indicating an older stellar population within the bulge. Fainter, more diffuse structures extend outwards from this core, with possible hints of a disturbed disk. The morphological structure displays only weak spiral arm features with a hint of blue color, suggestive of recent, but not exceptionally active, star formation. There's a slight irregularity visible in the disk, particularly on one side, which may be indicative of a minor gravitational interaction, or a possible merger event, based on the light scattering. Overall, it appears to be a relatively mature system, transitioning away from a purely disk-dominated morphology.
