The observed galaxy presents as a spiral galaxy with a relatively high degree of inclination with respect to our line of sight. The disk component appears to be the dominant feature, exhibiting discernible spiral arm structure. The spiral arms appear somewhat loosely wound. The central bulge is moderately sized, but relatively prominent. The galaxy does not appear to be undergoing any major merging events, nor are there obvious signs of significant tidal disruption, though some minor disturbances can't be ruled out given the image quality. The general morphology suggests ongoing star formation within the disk, evidenced by the blue tones associated with the spiral arms. A weak bar may be present across the center of the galaxy. The observed features suggest that the galaxy is not a purely quiescent system.
