The galaxy presents a generally smooth, elliptical morphology. It appears largely featureless, lacking any prominent spiral arms or a distinct disk structure. There is a concentrated central bulge of light, indicative of a high stellar density in the core region. The light emitted is concentrated in the redder wavelengths, which suggests an older stellar population. There are no signs of active star formation regions visible. There are no obvious signs of interaction with another galaxy, such as tidal tails or distorted morphology, although there is some minor asymmetry.
