The galaxy presents as a largely smooth, elliptical-like object with a concentrated central bulge. The core region exhibits a strong, yellowish-orange hue, which may indicate an older stellar population. This central region seems to fade outward into a diffuse greenish glow, possibly indicating the presence of some younger stars or ionized gas at greater distances from the center. The overall shape is somewhat elongated, tending toward a more spheroidal form rather than a highly flattened disk. There is no discernible evidence of major disturbances, strong tidal features, or ongoing major merger activity in this imagery. The galaxy's structure indicates that it is a relatively evolved system with a relatively low star formation rate.
