The galaxy appears to be a spiral type, seen at an oblique angle relative to our line of sight. The central bulge is prominent and exhibits a yellowish hue, suggesting an older stellar population and a relative lack of active star formation in the core. The disk surrounding the bulge shows evidence of spiral arm structure, although the arms are somewhat tightly wound. These arms are bluer in color, indicative of younger, hotter stars and ongoing star formation. The galaxy's overall color suggests a mix of stellar populations, with a dominant bulge component and a relatively active disk. No signs of major mergers or tidal disturbances are immediately apparent, although minor asymmetries or irregularities within the disk cannot be ruled out based on this image alone.
