The galaxy presents a largely smooth, elliptical morphology with a high degree of circularity. A prominent central bulge dominates the structure, displaying a bright, concentrated luminosity profile. No distinct spiral arms or bar features are discernible within the observed image. The galaxy exhibits a moderately red color, indicating a likely older stellar population with relatively low levels of ongoing star formation. There is no evidence of major tidal disturbances or ongoing merger activity, suggesting a relatively quiescent evolutionary state. 
