The galaxy presents a predominantly smooth, elliptical morphology, exhibiting a high degree of central concentration with a diffuse halo. The galaxy appears generally rounded. It shows an apparent lack of significant substructure or prominent spiral arms. The core displays a bright, yellowish-white hue, suggesting a population of older stars, with the light becoming redder towards the outer edges. There is some mild asymmetry in the outer regions. The overall color profile indicates that star formation may be relatively quiescent within the galaxy. A small amount of disturbance is possible.
