The galaxy appears to be a disk galaxy, oriented approximately edge-on relative to our line of sight. The central bulge is prominent, exhibiting a yellowish-orange hue, suggesting an older stellar population. There is a faint disk that extends horizontally from the bulge, appearing somewhat clumpy and less well-defined. There is evidence of minor disturbances in the galaxy's structure and a redder color in the central bulge, which indicates a region of older stars, or a more dust-obscured region. The galaxy also has some blue knots in the faint disk, indicating potential sites of active star formation. The outer regions of the disk fade considerably, resulting in a relatively compact appearance. The overall shape of the galaxy suggests it is relatively evolved, but still possesses some ongoing star formation activity.
