The observed galaxy presents as a relatively face-on spiral galaxy with a prominent central bulge. The bulge exhibits a smooth, concentrated brightness profile, suggesting a significant population of older stars. Moving outwards from the bulge, a disk structure is visible, although somewhat irregular in shape. Some features are visible in the disk suggesting possible spiral arm structures with moderate star formation. There are some indications of minor disturbances potentially from a small past merger. Overall, the galaxy exhibits a mix of smooth and featured morphologies, hinting at an evolving system. The galaxy appears relatively isolated. The bluer color suggests active star formation regions with some dust present.
