The galaxy presents as an elliptical or lenticular system, observed nearly edge-on. The central bulge exhibits a concentrated, yellowish hue, suggesting an older stellar population. Fainter bluish colors are present extending outwards, with the disk appearing somewhat asymmetric. There is a hint of dust absorption, but it is not extensive. There are faint signs of what may be minor tidal disruption, however, further investigation is needed to confirm this hypothesis. Overall, the galaxy displays characteristics of a relatively massive system with a low rate of current star formation.