The galaxy appears to be a relatively small, lenticular or early-type spiral galaxy. It exhibits a smooth, featureless morphology with a high degree of central concentration. There is a noticeable bulge, appearing nearly spherical, with a faint disk or flattened structure extending outwards. The disk presents a mottled appearance, likely due to unresolved stellar populations or dust lanes. The overall color is a muted blue, with a hint of yellow in the central bulge, indicating the presence of both younger and older stellar populations. There is no clear evidence of active star formation, such as HII regions or bright knots within the disk. No signs of a major merger are visible, though subtle asymmetry suggests a possible minor gravitational interaction in the past. The galaxy presents an apparent diameter of approximately 3 arcseconds.
