The galaxy presents a moderately inclined disk-like morphology. It exhibits a bright, concentrated central bulge that appears yellowish in color. This suggests a population of older, cooler stars dominating the core. The disk component displays a bluer hue, indicating the presence of younger, hotter stars and potentially ongoing star formation. The dust lanes within the disk are not clearly visible, but there is a slight mottled texture, suggesting some level of dust obscuration and potentially faint spiral arm structures. The galaxy appears relatively smooth, with no obvious signs of major mergers or tidal disturbances. Overall, it presents characteristics consistent with a late-type spiral galaxy, possibly an Sa or Sb type, at an intermediate redshift. Further spectroscopic analysis would be necessary to confirm its stellar population, star formation rate, and morphological classification.
