The galaxy presents as a lenticular or possibly an elliptical system, exhibiting a smooth, diffuse light distribution without readily apparent spiral arm structure. It is elongated in shape, with an aspect ratio suggesting a classification tending toward cigar-shaped. The central bulge is bright, with a concentration of light indicating an older stellar population. The outer regions exhibit a gradual decrease in luminosity, with some hints of a faint disk component. There is no evidence of active galactic nuclei activity or significant star formation. No signs of mergers or major disturbances are apparent. Overall, the morphology suggests an evolved system.
