The galaxy presents as a lenticular or possibly an elliptical galaxy seen edge-on, or at a highly inclined angle. The central bulge appears prominent and elliptical in shape, displaying a smooth, relatively uniform orange-red color profile, indicative of an older stellar population and low star formation activity. Faint blue tinges are present along the outer edges of the disk, which may suggest the presence of younger, hotter stars. The galaxy lacks any clear spiral arm structure or dust lanes. There are some indications of minor disturbances that may be due to a possible interaction or tidal effects. Overall, the galaxy exhibits a well-defined, elongated structure with a significant central concentration of light.
