The galaxy presents as a moderately luminous, disk-shaped system viewed at an oblique angle, suggesting it is close to edge-on. The central region exhibits a concentrated, bright bulge that appears relatively smooth and featureless. Surrounding the bulge is a faint, extended disk.  The disk appears to be composed of a mixture of young, blue stars and older, redder stellar populations. There is no clear spiral arm structure visible, the galaxy could be considered a lenticular galaxy. Based on the red color, the galaxy is expected to be quiescent and not actively forming many new stars. There is no sign of tidal disturbances that would suggest any significant ongoing merger events. 
