The galaxy presents as an edge-on spiral, with a prominent dust lane bisecting the elongated structure. The bulge appears to be rounded, with a relatively smooth texture, showing characteristics of an older stellar population. There is evidence of active star formation regions within the disk, indicated by the presence of bluer knots that are distributed throughout the galaxy. These areas contrast with the more yellowish hue of the bulge and inner disk regions. There is a faint hint of a possible minor tidal disturbance or asymmetry in the outer regions of the disk.
