The galaxy presents a generally smooth, elliptical morphology, with a high degree of central concentration.  It exhibits a luminous core, surrounded by a more diffuse halo. The light distribution appears to be relatively even, with no prominent spiral arms or distinct features. The color gradient suggests a population of older stars, with a possible contribution from dust extinction. There is a very slight indication of a possible minor disturbance.  The galaxy appears to be in a relatively quiescent state regarding star formation. The overall shape is not perfectly round, leaning more towards an intermediate elliptical form.
