The galaxy presents as a relatively edge-on disk galaxy. It exhibits a prominent central bulge, appearing more concentrated and yellowish in color compared to the surrounding disk. The disk component appears to be elongated, with a faint, diffuse light extending outwards from the bulge. There is a slight hint of dust lane absorption visible along the plane of the disk, although it is not particularly pronounced. The overall color gradient suggests a possible distribution of stellar populations, with the central bulge possibly dominated by older, redder stars and the disk containing a mix of both younger and older populations. The galaxy appears largely undisturbed, lacking any obvious signs of recent major mergers or tidal interactions. The bulge is appears to be a somewhat rounded. There is a lack of defined spiral arm structure.
