The galaxy presents as a diffuse, elliptical structure with a moderately smooth appearance. Its central region appears brighter and more concentrated than its outer regions. There is a suggestion of a disk-like structure, though subtle, implying it may be a lenticular galaxy. The galaxy does not appear to have any prominent spiral arms or bar structures. There may be evidence of a minor interaction or disturbance. The galaxy's color suggests a population of older stars. No active star-forming regions are readily apparent. The object’s morphology is largely smooth and not undergoing a major merger or violent starburst activity. Its roundness appears to be neither perfectly spherical nor particularly elongated.
