The galaxy presents a smooth, elliptical morphology. It appears largely featureless, lacking prominent spiral arms or a distinct bar structure. The core region exhibits a bright, concentrated luminosity, suggesting a significant stellar density. Moving outwards from the core, the luminosity gradually decreases. There is a slight flattening in the shape, deviating from a perfect sphere; it has a slight cigar shape. The color profile transitions from a yellowish core to a bluer halo. The galaxy does not appear to be undergoing any major merging events, though there is the possibility of minor disturbances in its structure.
