The galaxy presents as a lenticular or early-type spiral galaxy, with a smooth, bulge-dominated morphology. The object exhibits an elliptical shape, with a clear major axis and a minor axis, suggesting a disk-like structure viewed at an angle.

The color distribution across the galaxy appears relatively uniform. The central region shows a yellowish-white hue, indicative of an older stellar population. This color gradient suggests the presence of a bulge component composed of evolved stars. No distinct spiral arm structures or dust lanes are visible, further supporting its classification as a lenticular or early-type spiral galaxy. 

There is no strong evidence of active star formation within the galaxy, based on the lack of bright blue regions typically associated with young, massive stars. The overall appearance indicates a galaxy that is likely passively evolving. No prominent tidal features or distortions are apparent, suggesting it is not currently undergoing a major merger event.
