The galaxy presents as a spiral with a significant disk component viewed at an angle. The bulge region appears bright and concentrated, exhibiting a yellowish hue, indicative of an older stellar population. Spiral arms are clearly visible, appearing somewhat tightly wound around the central bulge. The arms exhibit a bluer coloration relative to the bulge, suggesting the presence of younger, hotter stars and ongoing star formation. There are likely two dominant arms. The overall morphology suggests a galaxy undergoing active star formation, particularly within its spiral arms. The shape is somewhat elliptical, with a moderate axis ratio. There is no visual evidence of a strong bar feature traversing the central region. The galaxy does not appear to be undergoing a major merger or experiencing significant tidal disturbances from interacting galaxies based on this image. The colors from the image may signify a redshift.
