The observed galaxy presents as an elongated, disk-like structure with a prominent central bulge. The galaxy appears to be viewed at a significant inclination. The central bulge exhibits a yellowish-orange hue, suggesting a population of older stars. The disk component shows a bluer color gradient moving away from the core, hinting at ongoing star formation within the spiral arms. The disk structure exhibits a degree of irregularity, possibly indicating past interactions or internal disturbances. There is no clear evidence of a major ongoing merger, though minor disturbances cannot be ruled out based on the available imagery. The overall morphology suggests a spiral or lenticular galaxy type.
