The galaxy presents as a lenticular or early spiral type, observed at a significant inclination. A bright, relatively compact central bulge is evident, surrounded by a prominent disk. The bulge exhibits a red-shifted color index. The disk displays hints of spiral arm structure, but these features are not well-defined. Two distinct, red-shifted areas can be seen at the ends of each side of the galaxy, suggesting that perhaps these are two arms, or areas where the disk is warping. There is a hint of a diffuse halo surrounding the galaxy.

Based on these visual features, the galaxy doesn't seem to display any signatures that would indicate that it is currently merging with another galaxy.
