The galaxy presents as an elliptical morphology, exhibiting a smooth and featureless structure. Its overall shape is largely spherical. A bright central bulge dominates the light profile, with luminosity gradually decreasing towards the outer regions. There is no clear evidence of spiral arms or a distinct disk component. The color is generally consistent across the galaxy's extent, with a slight shift towards redder hues suggesting an older stellar population. Signs of recent major merger activity appear to be absent. Small signs of disturbance are also not seen, suggesting a well-formed, isolated system.
