The galaxy appears as a relatively compact, disk-shaped system oriented approximately edge-on with respect to our line of sight. There is a central bulge of moderate luminosity, surrounded by a flattened disk component. Within the disk, the presence of star-forming regions is suggested by the clumpy, bluish-white concentrations of light, particularly concentrated towards the galaxy's center. The overall color profile indicates the presence of both older stellar populations (more yellow) and younger, hotter stars (more blue) signifying ongoing or recent star formation. The galaxy does not exhibit obvious signs of significant tidal disturbances or major mergers. The galaxy seems to be a normal disk galaxy without a bar. 
