The galaxy presents as a disk galaxy, observed nearly edge-on. A prominent central bulge is apparent, exhibiting a concentrated luminosity gradient. The bulge appears to be a yellow-gold hue, perhaps indicating an older stellar population. The disk component extends outward from the bulge. The disk shows a blue tinge, potentially indicative of more recent star formation activity. The dust lane is not readily visible, but the galaxy shows no sign of merging or interaction with other galaxies.
