The galaxy presents as a spiral type, viewed at a slight angle from face-on. Two prominent spiral arms are discernible, exhibiting a medium winding structure. A bar feature is present traversing the central region, although the strength of the bar is moderate. The bulge component appears moderate in size relative to the disk. There is no obvious evidence of significant tidal disturbances or major mergers. Some areas of star formation are present within the spiral arms, though not exceptionally pronounced. The color suggests an intermediate redshift, the bluer color indicates ongoing star formation activity and intermediate dust content. Overall, the galaxy appears to be a relatively undisturbed spiral with a well-defined disk structure.
