The galaxy appears as a lenticular or early-type spiral galaxy. Its morphology is characterized by a generally smooth and rounded light distribution, suggestive of a large bulge. There is a slight flattening but no distinct spiral arm structure is visible. 

The central region exhibits a concentration of light. Color gradients are subtle, with a tendency toward slightly bluer colors in the outer regions compared to the core, although this is not definitive. This may indicate ongoing, although weak, star formation activity outside of the central bulge. No clear evidence of a recent or ongoing major merger is apparent; the galaxy appears relatively undisturbed, though some possible minor tidal features cannot be ruled out.
