The observed galaxy presents an elongated, cigar-shaped morphology. The central region exhibits a concentrated, yellowish hue, suggesting a higher density of older stellar populations. Extending outward from this central bulge, fainter, bluish-white regions are visible, indicative of younger, hotter stars and potential ongoing star formation. The overall structure appears relatively smooth, with a lack of prominent spiral arms or distinct features. There is a slight asymmetry in the distribution of light, potentially suggesting minor gravitational interactions or internal disturbances, although no major merger events appear to be occurring. The gradual color gradient from the core to the outer edges indicates a shift in stellar population age and composition across the galactic disk.
