The galaxy presents as a somewhat elliptical structure with a dominant central bulge. The bulge exhibits a smooth, concentrated appearance, with a yellowish-white hue suggesting an older stellar population. There is a faint, diffuse disk component visible, though it lacks distinct spiral arm features in this image. The overall color index suggests a higher concentration of older stars. Given its apparent size and morphology, the galaxy is likely a massive system, and star formation is occurring at a modest rate. There is some indication of tidal disturbances or interactions with a neighboring galaxy. 
