The galaxy presents a well-defined disk structure, exhibiting a generally flattened morphology when viewed from this angle. The overall color profile indicates the presence of both older stellar populations, seen as redder hues, and younger, bluer stars, particularly in the disk regions. Spiral arm structures are discernible, though not exceptionally prominent. The central bulge appears moderate in size and luminosity compared to the disk, suggesting a relatively significant classical bulge component. There is evidence of a bar-like feature crossing through the center, further supporting the disk morphology. The disk component suggests ongoing or recent star formation, as indicated by the presence of regions of bluer light. The absence of any obvious strong tidal features or distortions indicates the galaxy is relatively isolated or has not experienced a major merger event recently, with most disturbances being considered minor. The galaxy is seen at a redshift value, which is consistent with a relatively distant object and informs of its motion away from our viewpoint.
