The galaxy presents a flattened, disk-like structure with an apparent spiral morphology. The central region exhibits a bright, concentrated luminosity, suggesting the presence of a significant bulge component. The spiral arms are prominent, displaying a tightly wound configuration.  Evidence of a bar-like structure bisecting the central bulge is apparent. The overall color suggests a mix of stellar populations, with a yellowish hue dominating the central regions and bluer tones tracing the spiral arms, indicative of ongoing star formation within these regions. The galaxy appears relatively isolated, showing no obvious signs of major interaction or merging events.
