Observed is a spiral galaxy at a redshift of approximately 0.089, indicating a considerable distance. The galaxy exhibits a distinct disk-like structure viewed at a high inclination, appearing elongated or cigar-shaped. The central bulge appears relatively prominent and shows a yellowish hue, indicative of an older stellar population. The disk component displays a bluer tint suggesting the presence of ongoing star formation, though without distinct spiral arm structures readily discernible in this image. There is no readily apparent evidence of a major merger event, although the possibility of minor tidal disturbances cannot be ruled out based on the morphology alone. The overall smoothness of the light distribution suggests that it has relatively homogenous distribution, possibly indicating that it is a relatively old system, that is not undergoing an intense burst of star formation.
