The galaxy presents a largely smooth, elliptical morphology. The central region exhibits a concentrated, reddish hue, possibly indicating an older stellar population or dust obscuration. Proceeding outwards, a diffuse, greenish glow surrounds the core, potentially suggesting the presence of younger, hotter stars or emission from ionized gas. The overall shape is generally ellipsoidal, appearing neither perfectly spherical nor highly elongated. No distinct spiral arms or bars are discernible, although some minor irregularities or disturbances are present in the outer regions. These disturbances could be the result of past minor merger events or tidal interactions. The galaxy demonstrates a general lack of significant star formation, suggesting a relatively quiescent state.
