The galaxy presents as a single, relatively smooth object with an elliptical morphology. The core exhibits a high degree of concentration of light. Progressing outwards from the core, the light distribution diminishes rather uniformly, with no evident spiral arm structures or prominent dust lanes. It appears more akin to an elliptical or lenticular type galaxy, with a notable absence of features indicative of active star formation. The overall color is slightly yellow, suggestive of a population of older stars. There may be very faint disk-like features, as the galaxy is not perfectly circular, but these are hard to distinguish and do not appear prominent. There does not appear to be any signs of major disturbances that might be caused by merging.
