The galaxy presents an elliptical morphology, appearing elongated and cigar-shaped. The central bulge exhibits a bright, yellowish hue, suggesting a significant population of older stars. Fainter, bluer regions are observed within the galaxy, possibly indicating areas of ongoing, albeit relatively modest, star formation activity. No distinct spiral arm structures are discernible. The overall structure suggests a galaxy that may be in the process of transitioning from a more actively star-forming state. The apparent smoothness of the light distribution indicates a lack of major disturbances or ongoing merger events. There is minor clumpy structure in the disk.
