The galaxy presents as a slightly elongated, lenticular form. Its central region exhibits a higher surface brightness, suggesting a concentrated nucleus or bulge. The light distribution appears relatively smooth, with little evidence of spiral arm structure or dust lanes. The overall color is slightly blue-ish, implying the potential presence of at least some young stars. The galaxy exhibits a relatively compact size, indicating an estimated diameter of around 4 kpc. There is no obvious indication of active galactic nucleus activity or major merger events, however there is the possibility of minor disturbances in the galaxy. The galaxy appears to be undergoing moderate levels of star formation.
