The galaxy presents as an edge-on spiral, exhibiting a flattened disk structure with a prominent central bulge. The bulge appears largely smooth and featureless, with a concentration of older, redder stars. The disk component shows a dust lane obscuring the central regions, suggesting a significant amount of interstellar medium. The overall color of the galaxy is relatively red, indicative of a stellar population that is somewhat evolved, with possibly ongoing, moderate star formation. There is evidence of some minor disturbances that appear to be external, suggesting potential interactions with another galaxy. 
