The galaxy presents as a slightly elliptical, disk-like structure with an apparent edge-on orientation. A prominent central bulge is observed, which is characterized by a concentrated region of light indicating a high stellar density and a potentially supermassive black hole. The disk is characterized by both smooth regions and some areas of substructure.

The color distribution suggests a mix of stellar populations. The central bulge presents as more yellow in color, consistent with older, redder stars. The disk appears more blue, especially along the edges, which suggests the presence of younger, bluer stars and ongoing star formation.
There also appears to be some minor disturbances in the structure of the galaxy, perhaps indicative of tidal interactions or past mergers. There might be very faint tidal arms.
