The galaxy appears to be a spiral type, presenting with a defined disk structure. The arms are quite tightly wound and difficult to discern individually. A central bulge is visible, although it does not appear to be the dominant feature of the galaxy, with a relatively subtle contribution to the overall light distribution. There may be a weak bar structure, with increased brightness in the center. No signs of any major or minor mergers appear to be present. There are regions of blue hues mixed within the spiral arms. The galaxy's overall color index suggests ongoing star formation within the disk, though perhaps not at an exceptionally high rate.
