The galaxy presents as an apparent edge-on spiral or disk galaxy, viewed at a relatively high inclination. A distinct dust lane is not readily discernible, although subtle variations in color and luminosity suggest possible obscuration within the plane of the disk. 

The central bulge region is visible and appears elongated along the major axis. The bulge exhibits a yellowish hue, possibly indicating an older stellar population. Fainter, bluish diffuse light extends outwards from the central region along the galaxy's major axis, suggestive of ongoing star formation within the disk. This could potentially include younger, bluer stars.

The image shows some indications of possible tidal disturbances. There is evidence of disrupted features emanating from the disk, and a second, smaller galaxy may be interacting with the primary galaxy.
