The galaxy presents a largely smooth, elliptical morphology. It exhibits a high degree of central concentration, appearing nearly spheroidal with very little evidence of a disk structure. There is a notable absence of spiral arms or bar features. The galaxy's light is dominated by redder wavelengths, suggesting an older stellar population with relatively low ongoing star formation. Color gradients are subtle across the galaxy, with a slightly yellower hue concentrated in the central bulge. There is no obvious presence of dust lanes or strong tidal features, suggesting a quiescent state and lack of recent major mergers. Close inspection does not reveal any distinct star-forming regions or HII regions within the galaxy. There is no strong evidence of an active galactic nucleus based on its smooth appearance. 
