The galaxy presents as a flattened, elongated structure, suggesting a disk galaxy observed edge-on. A central bulge is apparent, exhibiting a concentrated, luminous region. The galaxy appears relatively smooth, with little to no distinct spiral arm structure visible, although some disturbances appear present. It displays a color gradient from a yellowish central region to slightly bluer edges, hinting at possible differences in stellar populations. The shape also indicates that this could be a lenticular galaxy. The galaxy exhibits low levels of ongoing star formation. The galaxy is moderately massive. There is no apparent merging activity.
