The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a distinct central bulge characterized by a yellow-orange hue, suggesting an older stellar population. The surrounding disk appears less structured, displaying a smoother distribution of light with a faint greenish tint. The overall color profile suggests a limited ongoing star formation. The galaxy's elongated shape indicates a possible intermediate classification between a purely elliptical and a spiral galaxy, though no spiral arms are discernible within the resolution of the image. There is no visible evidence of major disturbances or ongoing mergers, implying a relatively quiescent evolutionary state.
